The galaxy presents as a diffuse, elliptical-like structure with a smooth overall appearance. The light distribution suggests a relatively homogenous stellar population throughout the main body, with a slight concentration towards the core. The color gradient across the galaxy is minimal. There is a potential hint of a minor disturbance in the morphology, possibly a faint tidal feature or a slight asymmetry in the outer regions, but the overall form appears largely undisturbed. The galaxy is relatively isolated, with no obvious signs of ongoing or recent major merger activity, although it could be in the early stages of an interaction. No clear spiral arm structures or prominent dust lanes are visible.
