The galaxy presents as a centrally concentrated elliptical morphology, exhibiting a smooth and primarily spheroidal structure. It displays a noticeable radial color gradient, shifting from a yellowish-white core to a more reddish hue in its outer regions, indicative of an older stellar population. The overall symmetry appears largely undisturbed, with no readily apparent signs of significant tidal interactions or ongoing major mergers. Subtle asymmetries may be present in the very faint outer halo.
