The galaxy presents a relatively smooth, elliptical morphology. It exhibits a bright, concentrated core region which appears yellowish-orange, suggestive of an older stellar population. The core gradually fades into a surrounding, more diffuse halo. The halo shows subtle color variations, hinting at possible differences in stellar populations or dust content within its structure. Faint, diffuse blue regions seem to be present, indicative of younger stars. The galaxy lacks any prominent spiral arm structure or significant dust lanes, further supporting its classification as an elliptical galaxy. Overall, the galaxy appears to be relatively isolated with no obvious signs of a major merger event, although minor disturbances can't be ruled out. The galaxy's shape is mostly circular, with a slight elongation.
