The galaxy presents a generally smooth, elliptical morphology. Its central region exhibits a yellowish-white hue, suggesting a population of older stars. There is a subtle color gradient, with the inner regions appearing more yellow and the outer regions trending slightly redder. The overall structure appears relatively undisturbed, showing no prominent signs of ongoing mergers or tidal interactions. A slight elongation is observed, deviating somewhat from a perfectly circular form, but not dramatically. No distinct spiral arm structures or prominent dust lanes are discernible. The galaxy appears as a fairly compact object.
