The galaxy presents as a centrally concentrated object with a smooth, relatively featureless appearance. It exhibits an elliptical morphology, appearing mostly round. There may be a faint disk, but the light is dominated by the bulge. The galaxy is characterized by a reddish-yellow hue, indicative of an older stellar population with less active star formation. There is no visible evidence of spiral arms or significant dust lanes. The galaxy shows no strong signs of ongoing mergers or major disturbances. There may be minor disturbances from smaller mergers, but they are not readily apparent.
