The galaxy presents as a largely smooth, elliptical form with a concentrated, bright central bulge. The light distribution appears to be relatively even, with a gradual decrease in intensity moving outwards from the core. Some subtle color gradients are observed; the central region exhibits a yellowish-white hue, suggesting an older stellar population. The outer regions appear slightly bluer, potentially indicating the presence of a younger stellar population. There appears to be a subtle extension or halo surrounding the main body, contributing to its overall size. There is no clear indication of spiral arms or significant dust lanes, supporting its classification as an elliptical galaxy. No signs of major ongoing mergers or tidal disturbances are immediately apparent, however a very slight lopsidedness suggests possible past interaction.
