The galaxy presents as a relatively smooth, elliptical-like structure. It exhibits a concentrated central bulge that appears yellowish, suggesting a population of older stars. The isophotes appear largely symmetrical and undisturbed, with no apparent signs of spiral arms or significant dust lanes. There's a hint of a more diffuse, fainter halo surrounding the core, suggesting a larger extent than the immediately visible bright region. The lack of prominent blue regions implies a relatively low rate of ongoing star formation. No merging activity or tidal disturbances are readily apparent in the immediate vicinity of the galaxy.
