The galaxy presents a generally smooth appearance with an elliptical morphology. The central bulge exhibits a concentrated luminosity profile with a yellowish-orange hue. Moving outward from the bulge, a subtle disk-like structure with a greenish tint is visible, although it is not clearly defined and appears relatively featureless. There is no strong evidence of spiral arms or significant dust lanes within the visible structure of the galaxy. The overall color suggests a population of older stars dominating the light output. There does not appear to be any major tidal distortions or signs of ongoing mergers. There is potentially minor evidence of a disturbance. The galaxy has a generally in-between shape, leaning towards round.
