The galaxy presents as a somewhat elongated, elliptical structure. It appears relatively smooth in texture, suggesting an older stellar population. The color gradient transitions from a bluish-white core to a redder outer halo, indicative of a change in stellar age and composition, with older, redder stars dominating the outskirts. A slight asymmetry is noticeable, hinting at a possible past interaction or minor disturbance. There is no clearly defined spiral arm structure or significant dust lane obscuration visible.
