The galaxy appears to be an elliptical galaxy. It exhibits a centrally concentrated luminosity profile, with brightness decreasing gradually toward the outer edges. The overall shape is somewhat ellipsoidal, but approaching circular, with a slight elongation along one axis. The core region displays a reddish hue, indicative of an older stellar population. Surrounding the core is a yellowish halo, and even further out there are regions showing blue and green emission. There is some evidence of minor disturbances in the outer regions of the galaxy, suggesting a possible past interaction or merger event, although the primary body of the galaxy remains relatively undisturbed. Based on the color gradient, star formation rates are generally low, with the outer regions having slight traces of star formation, while the core is quiescent. The galaxy is a substantial object, and its morphology is characteristic of a mature system, with most stars already formed and a stable structure.