NGC 407 is a spiral galaxy located in the constellation Cetus. It is approximately 70 million light-years away from Earth and is part of the Hubble Space Telescope survey. NGC 407 is notable 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 weakly barred structure. Observations of NGC 407 contribute to our understanding of galaxy formation and evolution, as well as the dynamics of star formation within spiral galaxies.