The galaxy presents as a single, concentrated luminous entity. Its overall form is elliptical, exhibiting a smooth, centrally concentrated light profile with a gradual decrease in brightness outward from the core. The nucleus is bright, with a soft yellow-white hue, indicating an older stellar population and minimal ongoing star formation. 

The overall color is indicative of a passively evolving system, with the relative brightness suggesting it is a massive galaxy. There are no clear signs of spiral arms, dust lanes, or active star-forming regions. The galaxy appears relatively undisturbed, showing no obvious signs of a recent major merger event or significant tidal interactions.
