The galaxy presents as a centrally concentrated object, displaying an elliptical morphology. It exhibits a relatively smooth light distribution, lacking prominent spiral arms or a well-defined disk structure. The color profile indicates a dominant population of older stars, with a yellowish-red hue. The galaxy appears relatively isolated, with no immediately obvious signs of major interactions or mergers. Faint blue regions on the periphery could be indicative of minor star formation activity, but the overall impression is that of a quiescent system. The isophotes appear generally regular and elliptical, with a slight elongation in one direction.
