The galaxy presents as an elliptical morphology, appearing largely smooth and well-defined. It exhibits a concentrated central bulge that transitions into a more diffuse halo. The color profile indicates a predominantly older stellar population, evidenced by the yellowish-red hue of the core region. There is minimal indication of spiral arm structure or significant dust lanes. The overall shape is nearly circular, suggesting a low degree of intrinsic flattening. Based on the limited color information, the star formation rate appears to be relatively low. Faint extensions or tidal features are not apparent, suggesting it is relatively isolated. There are no strong indications of an ongoing or recent major merger event.
