NGC_1022
NGC 1022 is a barred spiral galaxy located approximately 50 million light-years away in the constellation Phoenix. It was discovered by the astronomer John Herschel in 1834 and is classified as a type SBc galaxy, indicating its spiral structure with a central bar.
The galaxy has an apparent magnitude of about 12.5, making it faintly visible through small telescopes. NGC 1022 is part of a group of galaxies and is notable for its active star formation, which contributes to its bright, blue regions. Its study helps astronomers understand galaxy evolution and dynamics.