The galaxy presents a largely smooth, elliptical morphology. It exhibits a concentrated central bulge that transitions to a more diffuse outer halo. The galaxy appears to be relatively isolated, showing no obvious signs of major tidal disturbances or ongoing mergers, although a possible minor disturbance is not entirely ruled out. The light profile suggests a fairly evolved stellar population with a dominant redder color in the central region, indicative of older stars. Fainter, bluer regions extend outward from the core, possibly indicating some ongoing, albeit low, levels of star formation, or a younger stellar population in the outer regions. The overall shape is close to round.
