The galaxy presents as a centrally concentrated object with a relatively smooth and featureless appearance. It exhibits a generally elliptical morphology, appearing nearly round. The core region is notably bright, with a color that is slightly redder than the outer regions. Faint bluish tinges are visible in the outskirts of the galaxy, but the overall color profile suggests an older stellar population dominating its composition. There is no apparent evidence of major mergers or significant tidal disturbances affecting the galaxy's structure. However, subtle asymmetry in its light distribution cannot be ruled out, possibly indicating a minor interaction or internal dynamics.
