The galaxy presents a smooth, elliptical morphology. It exhibits a centrally concentrated luminosity profile, with the highest intensity light concentrated in the central bulge and gradually decreasing outwards. The galaxy appears relatively undisturbed, lacking prominent spiral arms or tidal features suggestive of recent major mergers. Its color is a somewhat uniform yellowish hue, suggesting a moderate population of older stars and a relatively low rate of ongoing star formation. No distinct dust lanes or prominent star-forming regions are visible. The overall appearance suggests a mature galaxy, likely composed predominantly of evolved stellar populations.
