NGC 581 is a spiral galaxy located in the constellation of Cetus. It is approximately 60 million light-years away from Earth and is part of the Hubble Space Telescope survey. The galaxy exhibits a well-defined spiral structure, making it an interesting subject for astronomers studying galaxy formation and evolution. This galaxy is classified as a type Sc spiral, characterized by its loosely wound arms and bright central bulge. NGC 581 is also notable for its active star formation regions, which contribute to its vibrant appearance. Observations of NGC 581 help scientists understand the dynamics of spiral galaxies in the universe.