NGC 102 is a spiral galaxy located approximately 200 million light-years away in the constellation Pisces. It is part of the Hubble Space Telescope catalog and is known for its distinct spiral structure, which is characterized by bright, well-defined arms that contain numerous stars and nebulae. This galaxy is classified as a type SAB, indicating that it has a weak bar structure in its center. Observations of NGC 102 contribute to our understanding of galaxy formation and evolution, as well as the dynamics of spiral galaxies in the universe.