The galaxy presents as a centrally concentrated, largely featureless elliptical. It exhibits a smooth, diffuse profile with a gradual decrease in surface brightness from the core outwards. The central region displays a yellowish-white hue, suggestive of an older stellar population. Moving away from the center, a subtle shift towards a bluer color is observed, potentially indicating some ongoing, albeit modest, star formation activity in the outer regions. The overall shape is somewhat elongated but still roughly circular, exhibiting an "in-between" morphology that is neither perfectly round nor distinctly cigar-shaped. There are no prominent spiral arms, dust lanes, or other features typically associated with disk galaxies. The galaxy appears relatively undisturbed, showing no signs of a recent major merger event, although subtle irregularities in the outer halo might indicate past minor interactions.
