The galaxy presents a largely smooth, elliptical morphology. The light distribution appears centrally concentrated, with a gradual fading towards the outer regions. Color gradients are subtle, with a slightly bluer hue in the immediate surrounding area and a generally redder tone within the concentrated center. The overall appearance indicates a relatively evolved system with likely minimal ongoing star formation. There is no discernible evidence of spiral arms, dust lanes, or any major mergers or tidal disturbances. The galaxy shows a round structure, with no evidence of asymmetry.
