The galaxy presents as a relatively smooth, centrally concentrated object. The dominant morphology appears to be elliptical, with a high degree of radial symmetry. The core region exhibits a noticeable reddening, suggesting a population of older stars. The outer regions show bluer colors, possibly indicating a small amount of ongoing star formation. There is no obvious presence of spiral arms or a distinct disk structure. No signs of major mergers or significant tidal disturbances are apparent, though a very slight asymmetry to the outer halo might suggest a minor interaction in the past. The galaxy's shape appears somewhere between round and elliptical, perhaps slightly leaning towards the latter. The size is somewhat small and appears to be somewhat distant given the colors.
