The galaxy presents as a fairly smooth, elliptical-like structure. It appears quite round. The galaxy exhibits a color gradient, with the core region appearing more yellow/red, suggestive of an older stellar population, while the outer regions appear slightly bluer. There is no strong evidence of significant spiral arm structure or prominent dust lanes. The overall light distribution is relatively even, with a centrally concentrated bulge. There are no immediately obvious signs of major merging activity or significant tidal disturbances, though a very subtle irregularity in the outer halo cannot be ruled out.
