The galaxy presents a largely smooth morphology, with minimal discernible substructure. It appears elliptical in shape, approaching circularity, with a slight elongation. The central region exhibits a higher concentration of light, gradually decreasing in intensity towards the outer edges. The color profile suggests a dominant population of older stars, indicated by the reddish-yellow hue in the core, transitioning to a slightly bluer tint in the outer regions, potentially indicating some ongoing, though subdued, star formation. There is no evidence of spiral arms or a prominent disk structure. No signs of major mergers or significant tidal disturbances are apparent. The overall appearance suggests a relatively evolved, quiescent system.
