The galaxy presents as a predominantly smooth, elliptical-like structure. It exhibits a concentrated central bulge, which suggests a high stellar density in the core. The color gradient transitions from a bright, yellowish core to a more subdued, reddish outer halo, indicating a potential difference in stellar populations and ages, with older, redder stars dominating the outskirts and a more mixed population in the core. There's no visible spiral arm structure or distinct dust lanes, further supporting the classification as an elliptical galaxy. The roundness of the galaxy suggests that it is an early-type galaxy that has undergone substantial dynamical relaxation. Overall, it presents as a well-formed, relatively undisturbed galaxy.