NGC 151 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 {Sloan Digital Sky Survey}. NGC 151 has a diameter of about 100,000 light-years and contains billions of stars. This galaxy is classified as a type Sc spiral galaxy, which means it has well-defined spiral arms and a prominent central bulge. NGC 151 is also notable for its active star formation, making it an interesting subject for astronomers studying galaxy evolution and structure.