The galaxy presents as a relatively smooth, centrally concentrated object with a noticeable elliptical morphology. There is minimal evidence of spiral arms or significant disk-like structures. The light profile appears to diminish gradually from the core outward. The color is reddish-yellow, suggesting a stellar population dominated by older stars and potentially a lower rate of ongoing star formation. There might be a slight indication of minor disturbance in the outer regions, though no clear merger events or strong tidal features are visible. The overall appearance implies a massive galaxy with potentially a large spheroidal component.
