The galaxy presents as a smooth, elliptical object. It exhibits a relatively high degree of ellipticity, appearing cigar-shaped with a major axis significantly longer than its minor axis. The color gradient suggests a redder core region, potentially indicating an older stellar population concentrated in the center. The outer regions appear bluer, hinting at the presence of younger stars or a small amount of ongoing star formation, though it seems largely quiescent. There is no evidence of distinct spiral arms or significant dust lanes. No signs of any major disturbances.
