The galaxy appears as a relatively smooth, elliptical-shaped structure. Its light profile is centrally concentrated, with a gradual decrease in intensity towards the edges. The galaxy exhibits a yellowish-red hue, suggesting an older stellar population with a relative lack of ongoing star formation. There are subtle hints of asymmetry in the outer regions, which might be indicative of minor tidal interactions or past merger events. There is no definitive spiral arm or bar structure visible. The estimated size indicates that it is a moderately sized galaxy.
