The galaxy presents as a luminous, elliptical object. It is characterized by a relatively smooth and centrally concentrated light distribution, suggestive of an early-type morphology. There is no immediately apparent spiral arm structure or prominent dust lanes. Its overall color appears relatively red, possibly indicating a population of older stars and reduced current star formation activity. The galaxy exhibits a moderate degree of roundness. There are slight indications of some minor disturbances in the surrounding area, but no clear signs of ongoing or recent major merger events. The mass estimate is in the range of a large galaxy.
