I’ve viewed it quite a few times — here’s an incomplete list of observations. Obviously aperture makes a huge difference as the individual components are only mag ~16.7 and 16.9. As far as splitting the pair in a 10” (seeing both simultaneously) I seriously doubt it, though someone with excellent vision, seeing and transparency might be able to glimpse it as a single blurry object.
The nearby bright galaxy is NGC 3079.
Steve
82" (5/4/19): at 613x; very clean split with both components easily visible continuously. The southern "B" image appeared a few tenths of a magnitude brighter.
48" (4/24/25): viewed at 813x and 1084x. At 6" separation, the pair was widely split at this high power and visible continuously as sharp points. The southern "B" lensed image was clearly brighter.
48" (4/18/15): both mag 16.7/16.9 components easily visible nearly continuously at 697x. The southern component was clearly slightly brighter, although delta V is only 0.2. At 6" separation, the pair is relatively widely split. The lensing foreground galaxy 2MASX J10012087+5553496 = YGKOW G1, which has a redshift of z = 0.356 (light-travel time 3.9 Gyr), wasn't seen.
48" (4/6/13): the mag 16.5/16.7 components were cleanly split at 488x, though easier at 610x. The southern "B" component was slightly brighter.
48" (4/15/10): the gravitationally lensed Double Quasar was very easily split in the 48" at 700x. At this magnification, the two components, separated by 6" were widely split with lots of clean space between the quasar images. The individual components appeared as perfectly sharp mag 16.5 and 16.7 stars oriented ~N-S, with the slightly brighter "B" component (delta V = 0.25) to the south.
18" (2/14/10): although it was not difficult to starhop over to the position from NGC 3079, the double quasar was glimpsed at 280x as a slightly fuzzy 16th magnitude star with averted vision. The components seen only as a single glow (perhaps one component or the other). Located just west of a group of mag 14-15 stars and 1.1' NW of a mag 14.6 star.
17.5" (4/15/99): the field of the gravitationally lensed twin quasars was easily found by quickly starhopping 15' NNW from NGC 3079 to a small asterism of six mag 14-15 stars. The double quasar is situated 1.0' NW of a mag 14.5 star in the NW corner of the asterism. At 280x and 380x an extremely faint 16th magnitude nebulous glow was intermittently visible . Appeared slightly fuzzy but the individual mag 16.7 components, which are separated by just 6", weren't resolved.