The galaxy presents as a primarily smooth, elliptical structure. The light profile appears centrally concentrated, with a bright, unresolved core that likely hosts a supermassive black hole. Moving outwards, the light intensity gradually decreases with no prominent spiral arms or distinct features immediately visible.

There is a slight elongation of the galaxy along a major axis, hinting at an elliptical morphology that is in-between perfectly round and cigar shaped. The outer regions of the galaxy exhibit a subtle color gradient, shifting from a yellowish-white hue near the core to a slightly redder tint at the periphery, potentially indicating an aging stellar population in the outer halo. The general symmetry of the light distribution suggests a relatively undisturbed system, free from recent major merger events. Minor disturbances or interactions cannot be fully excluded due to the limited image resolution.
