The galaxy presents a primarily smooth morphology, suggestive of an elliptical galaxy. It exhibits a notable central concentration of light, indicating a likely bulge component. The overall shape appears moderately elliptical. Color gradients within the galaxy are subtle, with a generally yellowish hue that shifts towards slightly redder tones in the outermost regions, suggesting a population of older stars dominating the light output. There is little evidence of spiral arms or significant dust lanes, further supporting a classification as an early-type galaxy. No signs of significant tidal disturbances or ongoing mergers are visible.
