NGC 1762
NGC 1762 is a spiral galaxy in the constellation of Orion. Its velocity with respect to the cosmic microwave background is, which corresponds to a Hubble distance of. However, 10 non-redshift measurements give a farther mean distance of. It was discovered by German-British astronomer William Herschel on 8 October 1785.
NGC 1762 has a possible active galactic nucleus, 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.