The galaxy presents a generally smooth and centrally concentrated morphology. Its shape is observed to be somewhat elliptical, displaying an intermediate axial ratio, not appearing perfectly round or highly elongated. The light distribution indicates a prominent bulge component, brighter and more concentrated towards the center. The galaxy exhibits colors generally consistent with an older stellar population. The lack of strong, distinct features, such as spiral arms or prominent dust lanes, suggests a relatively evolved system. Evidence of a minor interaction or disturbance cannot be ruled out, though there is no significant sign of major merging activity. The overall appearance aligns with what is typically observed in early-type galaxies.
