NGC 587 is a spiral galaxy located in the constellation of Cetus. It is approximately 80 million light-years away from Earth and is part of the Hubble Space Telescope observations, which have provided detailed images of its structure. This galaxy is notable for its bright core and well-defined spiral arms, which are rich in stars and interstellar gas. NGC 587 is classified as a type Sc spiral galaxy, indicating a moderate degree of winding in its arms. Its study contributes to our understanding of galaxy formation and evolution in the universe.