The galaxy presents as a relatively smooth, elliptical-like structure. It exhibits a bright, concentrated central region indicative of a significant galactic nucleus. The galaxy shows a gradual decrease in luminosity from the core outwards, without any distinct spiral arm structures or prominent dust lanes visible. The color profile suggests an older stellar population, appearing more yellow/red in the core, transitioning to a slightly bluer hue in the outer regions of the galaxy. There are no obvious signs of major ongoing mergers or tidal disturbances, suggesting a relatively undisturbed evolutionary history. Overall, the galaxy appears as a well-defined, early-type system with a dominant spheroidal component.
