The galaxy presents a largely smooth, elliptical morphology, exhibiting a concentrated central bulge. Its color gradient suggests a redder core, possibly indicating an older stellar population. The outer regions appear slightly bluer, which may indicate the presence of some younger stars or ongoing, albeit low, levels of star formation. There's a subtle hint of asymmetry in the overall shape, which could be due to a minor gravitational interaction or internal dynamics. The galaxy appears relatively undisturbed with no clear signs of major merging events.
