The galaxy presents as a relatively smooth, centrally concentrated object. It exhibits a flattened, elliptical morphology, tending towards an intermediate spheroidal shape, and is not perfectly round. There is no discernible evidence of spiral arm structure. The galaxy's color is consistent with an older stellar population, appearing redder overall than galaxies with ongoing active star formation. There are no obvious signs of recent or ongoing major mergers or significant tidal disturbances, although minor irregularities or subtle disturbances cannot be entirely ruled out.
