The galaxy presents as a relatively smooth, centrally concentrated elliptical. It exhibits a moderate ellipticity, appearing more in-between round and cigar-shaped. There are no visually apparent spiral arm structures or significant dust lanes. The color profile suggests a population of older stars, with a yellowish to reddish hue dominating the central regions. There is no indication of a recent major merger event or significant tidal disturbances and the rate of star formation is likely low. The galaxy's overall structure appears undisturbed, indicating a relatively quiescent evolutionary state.
