The galaxy presents a generally smooth, elliptical morphology with a concentrated central bulge. The light profile appears relatively uniform, suggesting a lack of significant spiral arm structure or prominent dust lanes. There is a slight elongation, the galaxy is round, but not perfectly so. The core exhibits a yellowish-white hue, potentially indicating an older stellar population dominating the central region. The outer regions of the galaxy display a subtly greenish tint, which could be indicative of ongoing, though subdued, star formation. Overall, the galaxy's structure appears relatively undisturbed, with no obvious signs of major mergers or tidal interactions, although some minor disturbance is possible.
