NGC 3077
NGC 3077 is a small spiral galaxy located approximately 8.1 million light-years away in the constellation Ursa Major. It is part of the M81 Group, which includes several other galaxies, such as M81 and M82. NGC 3077 has a diameter of about 30,000 light-years and is notable for its irregular structure and active star formation.
Discovered by the astronomer William Parsons in 1850, NGC 3077 is often studied for its interactions with neighboring galaxies. These interactions can lead to the formation of new stars and influence the galaxy's shape over time. Its proximity to other galaxies makes it an interesting subject for astronomers exploring galactic dynamics.