The galaxy presents as a primarily smooth, elliptical structure, exhibiting a high degree of central concentration. The core region appears bright and slightly yellow, suggesting a population of older stars. There is a subtle color gradient, with the outer regions appearing somewhat redder, indicative of a relatively quiescent star formation rate. No distinct spiral arms or bar structures are discernible. The overall morphology implies a galaxy undergoing, or having completed, a transition towards a more passively evolving system. There is no obvious evidence of recent major mergers or significant tidal disturbances. The galaxy's apparent roundness suggests it is viewed close to face-on.
