The galaxy presents as a relatively smooth, elliptical structure. It exhibits a somewhat elongated morphology, appearing more "in between" round and cigar-shaped rather than perfectly circular. The color profile suggests a dominant population of older stars, emitting primarily in the redder wavelengths with some blue light emission towards the center. There is no clear evidence of significant spiral arm structure or dust lanes, suggesting a later-type galaxy where star formation is relatively quiescent. A minor asymmetry is observed, potentially indicating a past interaction or minor disturbance. There are no prominent tidal tails or other clear indicators of an ongoing major merger.
