The galaxy appears to be an elliptical galaxy with a bright, concentrated core. The central region exhibits a high degree of smoothness, transitioning to a more diffuse halo. The isophotes are generally rounded, though with subtle deviations suggesting some tidal disturbance. Faint, extended features are observed, possibly indicative of a minor merger event or tidal interactions with other galaxies. The overall color index suggests an older stellar population with a redder hue in the central region. Some minor dust lanes or features are visible, lending support to it being in the midst of a merger event.