This galaxy presents as a somewhat elongated, elliptical structure with a high degree of central concentration. The overall color profile suggests a relatively older stellar population, particularly in the central bulge, which exhibits a yellowish-white hue. The outer regions display a slightly bluer tint, hinting at the presence of younger, hotter stars, perhaps indicative of ongoing, albeit subdued, star formation activity. There are no discernible spiral arms or distinct dust lanes, which supports the classification as an elliptical galaxy. The galaxy appears relatively undisturbed, with no obvious signs of recent major mergers or tidal interactions, although a faint asymmetric extension on one side may indicate minor gravitational disturbances.
