The galaxy presents as a relatively smooth, elliptical-like structure. Its overall color is yellowish, suggesting an older stellar population with fewer young, blue stars. There is little evidence of spiral arms or significant dust lanes, reinforcing its classification as a spheroid galaxy. The galaxy appears compact and relatively undisturbed, with no obvious signs of tidal interactions or ongoing mergers. It displays a well-defined central concentration of light, hinting at a possible central supermassive black hole. 
