The galaxy presents a primarily smooth, elliptical morphology. It exhibits a concentrated, bright central bulge, decreasing in luminosity towards its outer regions. There is some evidence of a slight disk-like component extending from the central bulge, indicating that it is not a pure elliptical galaxy. The overall color is predominantly yellow, suggesting an older stellar population with a lower rate of active star formation. A faint disturbance or tidal feature is observed extending from one side of the galaxy, which could be indicative of a past interaction or minor merger event. The galaxy's shape appears relatively round, with only a slight deviation from perfect circularity.
