The galaxy appears to be a relatively smooth, elliptical system with a concentrated central bulge. The light distribution is highly concentrated. There are no strong indications of spiral arm structure or significant dust lanes. It exhibits a roughly circular morphology. A slight asymmetry is noted in the light distribution, with a possible tidal feature or minor disturbance visible on one side, suggesting a possible interaction. The color is generally redder, indicative of an older stellar population with little ongoing star formation.
