The galaxy presents a relatively smooth, elliptical morphology. Its central region displays a bright, concentrated core, suggestive of a high stellar density. The galaxy exhibits a color gradient, appearing more yellow in the center, which could imply an older stellar population dominating the core. The outer regions fade gradually, indicating a less concentrated distribution of stars compared to the core. Faint indications of a diffuse halo are possibly visible, surrounding the main galactic body. There is no clear evidence of spiral arms, bars, or significant dust lanes. The overall appearance suggests a relatively evolved system with minimal ongoing star formation. Small asymmetric features are visible, perhaps minor tidal disturbances.