The galaxy presents as a singular, relatively smooth and elliptical light distribution. The core appears brighter than its surrounding halo, suggesting a concentration of stars towards the center. There is a subtle gradient in brightness moving outward from the core. The galaxy does not exhibit any clear spiral arm structure or strong tidal features indicative of recent major mergers or disturbances. The overall shape is generally circular, showing a slight deviation from perfect sphericity. There may be subtle hints of minor irregularities in the outer regions, potentially indicating minor interactions or internal processes. Its red color suggests an older stellar population with minimal current star formation.
