The galaxy presents a largely smooth, elliptical morphology with a high degree of central concentration. The core region exhibits a bright, yellowish-white color, suggestive of an older stellar population. The isophotes are generally circular, with minimal apparent distortion or tidal features, indicating a relaxed dynamical state. There is a faint, diffuse halo extending outwards from the central region, fading into the background sky. The galaxy appears relatively isolated, showing no obvious signs of recent or ongoing major mergers. Overall, the galaxy appears to be a massive early-type galaxy with little current star formation activity.
