The galaxy presents as a centrally condensed object with a smooth, elliptical morphology. There is little to no visible substructure, such as spiral arms or a prominent bar. The color profile suggests a relatively homogeneous stellar population, with a slightly bluer hue at the outer edges, suggestive of ongoing, but not substantial, star formation. The galaxy is roughly circular in appearance. There is no evidence of tidal features, major mergers or disturbances.
