The galaxy presents as an elliptical or lenticular type. It exhibits a smooth, centrally concentrated light distribution, with a gradual decrease in surface brightness outward from the core. The core region appears yellowish-white, suggesting a population of older stars. The overall color of the galaxy shifts towards redder hues in the outer regions. There is a slight flattening of the galactic disk. No spiral arm structures are discernible in this imaging. There is no visual evidence of a current merger or significant tidal disturbances. The isophotes appear fairly regular and elliptical, with a possible minor deviation.
