The galaxy appears to be elliptical in morphology, with a smooth and relatively featureless structure. Its overall color is slightly yellowish-white at the center, indicating an older stellar population. The outer regions display a faint bluish tint, possibly suggestive of more recent, albeit modest, star formation. There is no evidence of a distinct disk or spiral arms; the light is diffusely distributed. The galaxy exhibits a concentrated core region, which gradually fades into the surrounding halo. No signs of ongoing major merger activity are detected. Minor irregularities in the outer regions could imply past interactions or minor disturbances. The galaxy presents a roughly circular profile.
