The galaxy presents a generally smooth, elliptical morphology. The light distribution suggests a centrally concentrated spheroid, with a gradual decrease in luminosity extending outwards. The central region exhibits a yellowish hue, potentially indicating an older stellar population and/or dust obscuration. There is a slight elongation observed, deviating from a perfectly circular shape. The absence of discernible spiral arms or distinct features points towards a galaxy lacking significant ongoing star formation. There are no obvious signs of a major merger or strong tidal interactions. A subtle asymmetry might be present in the outer regions, suggestive of minor past interaction or internal processes. The overall impression is of a relatively quiescent, evolved galaxy.
