The galaxy presents an elliptical morphology, appearing smooth and relatively featureless at this resolution. It exhibits a concentrated central bulge with a decreasing intensity gradient towards its outer regions. The core appears to be a warm hue, possibly indicative of an older stellar population. The outer regions display a greenish-yellow color, which could signify a slightly younger population of stars or some active star formation, though subdued. There is no distinct spiral arm structure or bar visible. The galaxy appears relatively undisturbed, with no signs of major mergers or tidal disruptions. The overall shape is somewhat flattened, suggesting a rotating system, though the smoothness implies a lack of significant ongoing star formation in a well-defined disk.
