The galaxy presents as a centrally concentrated object, with a generally smooth appearance. The overall shape is elliptical, although it appears slightly elongated. There is a suggestion of a disk component, but the galaxy is dominated by its bulge-like structure. No distinct spiral arms or other major features are apparent. The color profile indicates a population of older stars, with a possible redder central region and slightly bluer outer regions. The galaxy appears relatively isolated, without evidence of ongoing major mergers, although minor disturbances cannot be ruled out.
