The galaxy presents as a centrally concentrated object with a largely smooth morphology. It exhibits a noticeable color gradient, transitioning from a yellowish-white core to a bluer halo. The galaxy's overall shape is generally elliptical, with the ratio of major to minor axes being approximately 3:2. There is little evidence of spiral arm structure or significant dust lanes. The outer regions show a slight fuzziness, potentially indicative of a stellar halo or tidal features, though no clear signs of ongoing major mergers or strong interactions with nearby galaxies are apparent. The light distribution suggests a dominant bulge component.
