NGC 391
NGC 391 is an unbarred lenticular galaxy located in the constellation Cetus. Its velocity with respect to the cosmic microwave background is, which corresponds to a Hubble distance of. Additionally, one non-redshift measurement gives a farther distance of. It was discovered by American astronomer George Bond on January 8, 1853. It was described by Dreyer as "faint, small, mottled but not resolved."