IC 758
IC 758 is a barred spiral galaxy in the constellation of Ursa Major. Its velocity with respect to the cosmic microwave background is, which corresponds to a Hubble distance of. However, two non-redshift measurements give a much farther distance of. It was discovered by American astronomer Lewis Swift on 17 April 1888.
The SIMBAD database lists IC 758 as 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.