The galaxy presents an overall elliptical morphology, appearing somewhat flattened along its major axis. Its light distribution exhibits a centrally concentrated profile, with a bright core that gradually diffuses outward. The primary coloration of the galaxy is a pale blue, indicating the potential presence of younger stellar populations or ongoing star formation activity, particularly within the central region. There is a subtle color gradient observed from the central region to the outer edges, suggestive of possible variations in stellar populations or dust content across the galactic body. Faint extensions or tidal features are not readily apparent in this view, suggesting a relatively undisturbed system without recent major mergers. However, there are some minor disturbances that can be observed.