NGC 5475 is a spiral galaxy located in the constellation Canes Venatici. It is part of the Virgo Cluster and is approximately 70 million light-years away from Earth. This galaxy is notable for its bright core and well-defined spiral arms, which are characteristic features of spiral galaxies. Discovered by the astronomer William Herschel in 1788, NGC 5475 is often studied for its structure and star formation activity. It is classified as a type Sc spiral galaxy, indicating a loose spiral structure with prominent arms. Observations of NGC 5475 contribute to our understanding of galaxy formation and evolution.