The galaxy presents a primarily smooth, elliptical morphology. It is characterized by a central concentration of light, indicating a prominent galactic nucleus or bulge. The overall color gradient suggests an older stellar population, with a yellowish-white hue dominating the central region. The galaxy does not appear to exhibit prominent spiral arms or significant dust lanes, reinforcing its classification as an elliptical galaxy. There might be a slight asymmetry or minor disturbance in the outer regions, which warrants further investigation into potential past mergers or interactions, though the primary impression is one of a settled, relatively undisturbed system. The elongated shape suggests a level of ellipticity between a circular and a cigar-shaped structure.
