NGC 1055 is a barred spiral galaxy located approximately 52 million light-years away in the constellation Phoenix. It is part of the NGC 1055 group, which includes several other galaxies. NGC 1055 has a bright central bar structure and exhibits a prominent disk of stars and gas. The galaxy is notable for its relatively high surface brightness and is classified as a type SBbc, indicating its spiral structure with a central bar. Observations of NGC 1055 contribute to our understanding of galaxy formation and evolution in the universe.