The galaxy presents a largely smooth morphology, appearing elliptical in shape with a moderate degree of ellipticity. It exhibits a concentrated central bulge that dominates the overall light profile. The color is predominantly redder and yellower in the central region, indicative of an older stellar population. The outer regions show a subtle bluer tint, suggesting the presence of a younger, albeit sparse, stellar population. There is no apparent spiral structure, nor are any signs of major tidal disturbances or ongoing mergers readily visible. Minor disturbances might be present, but are difficult to resolve from this view. Overall, the galaxy appears to be a relatively evolved system with minimal ongoing star formation activity.
