The object presents as an elliptical galaxy of intermediate apparent size, possessing a bright, concentrated central bulge region that dominates its overall morphology. The galaxy's color profile indicates a relatively older stellar population in the central region. The outer regions of the galaxy are less defined and exhibit a bluer tint, potentially indicating the presence of younger stars or ongoing star formation, although this is somewhat subtle. There are indications of subtle disturbances or asymmetry in the galaxy's morphology. There are no clearly defined spiral arms or a well-defined disk structure visible. The light distribution appears relatively smooth, but there is some indication of minor irregularities in the outer halo, suggestive of possible past interactions or mergers. Overall, this appears to be an elliptical galaxy exhibiting some features potentially indicative of a recent minor merger or interaction, although the dominant characteristic is that of a relatively smooth, centrally concentrated elliptical galaxy.
