The galaxy presents as a relatively smooth, elliptical object. There is a bright central bulge, slightly elongated in shape. The core of the bulge exhibits a yellowish-white hue, suggesting a population of older stars. Moving outward from the core, the color gradient shifts towards a reddish-orange, which could indicate cooler stellar populations or dust obscuration. The galaxy appears mostly undisturbed, lacking any obvious signs of recent major mergers or tidal interactions. The overall morphology points towards a galaxy that has largely completed its star formation, with a lower star formation rate currently ongoing.
