NGC 1077 is a barred spiral galaxy located approximately 50 million light-years away in the constellation Phoenix. It is part of the Hubble Sequence of galaxy classifications and is known for its distinct spiral arms and central bar structure. This galaxy is notable for its interactions with nearby galaxies, which can influence its shape and star formation activities. Observations of NGC 1077 contribute to our understanding of galaxy evolution and the dynamics of galactic interactions in the universe.