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Leo 1 is a dwarf galaxy, part of our Local Group of galaxies, which based on Wikipedia and other websites, is some 800,000 + light years from us. Its estimated diameter is 2000 light years and the dwarf galaxy has an estimated mass of 25 million solar masses. By contrast, estimates of the mass of our galaxy are 1.5 trillion solar masses and 87,000 light years across (but about 1000 ly thick)
Leo 1 was discovered only in the 1950s, from Palomar Observatory's 48" camera plates. Most stars in Leo 1 are estimated to have formed between 7 million and 1 million years ago, when star formation stopped. One hypothesis is that a close approach to our galaxy stripped off the gas clouds needed for further star formation. It is believed that Leo 1 contains a super massive central black hole and that the dwarf galaxy is dominated by dark matter. Star composition is largely hydrogen and helium, which indicates ancient formation, of interest for galaxy evolution work. Leo 1 is therefore an object being studied in some detail.
Leo 1 has no discernible structures such as spiral arms. Low surface brightness makes it hard to observe without a large telescope, though imaging by medium sized telescopes reveals the dwarf galaxy as a scatter of stars visually somewhat similar to open star clusters. My image with a 30mm objective and 150mm focal length shows the dwarf galaxy as a faint elliptical smudge at 12 o'clock to Regulus in the constellation of Leo. You may have to turn up screen brightness to see it.
Dwarf mini, 30/150mm, EQ mode, 148 exposures @ 30 seconds each, gain 60, stacked in DwarfVision.