NGC 1578
NGC 1578 is a spiral galaxy in the constellation of Dorado. Its velocity with respect to the cosmic microwave background is, which corresponds to a Hubble distance of. It was discovered by British astronomer John Herschel on 27 December 1834.
NGC 1578 is an active galactic nucleus candidate, i.e. it has a compact region at the center of a galaxy that emits a significant amount of energy across the electromagnetic spectrum, with characteristics indicating that this luminosity is not produced by the stars.