The galaxy presents as a somewhat elliptical, fairly concentrated object with a smooth overall appearance. The light profile suggests a central bulge that dominates the morphology. There is a subtle color gradient, with the core appearing more yellow/red in hue, likely indicating an older stellar population. Fainter, bluer extensions emanate from the central region, possibly indicative of a weak disk component or tidal features resulting from past interactions. No distinct spiral arms or prominent dust lanes are visible. The galaxy appears relatively undisturbed, exhibiting a symmetrical shape. There are no apparent signs of major mergers or significant tidal distortions. Overall, the galaxy seems to be a relatively evolved system, potentially residing on the red sequence.
