The galaxy presents as a fairly smooth, elliptical structure. The central region exhibits a high surface brightness, indicating a significant concentration of stars. The light distribution appears mostly spheroidal, with a gradual decrease in intensity from the core outwards. There is a suggestion of a slight disk or other minor feature present, but overall the galaxy appears relatively featureless and dominated by its bulge component. No major distortions or tidal features are apparent, suggesting that the galaxy has not undergone a recent major merger. The galaxy exhibits colors that are relatively consistent across the body, with a slight bluer hue visible. This suggests the presence of some young stars, but the galaxy is dominated by an older stellar population. Star formation appears to be occurring at a low rate. Based on its morphology, it can be classified as an early-type galaxy.
