The galaxy presents as a primarily smooth, elliptical morphology, lacking prominent spiral arm structures. The central region exhibits a concentrated luminosity gradient, appearing bright and yellowish, suggesting a significant population of older stars. The outer regions show a gradual decrease in surface brightness and a slightly bluer hue, hinting at the presence of younger stellar populations. The galaxy displays a moderate degree of ellipticity. There is no evidence of major tidal disturbances or ongoing mergers from visual inspection. The overall color profile indicates a galaxy with a moderately evolved stellar population and a relatively low rate of current star formation.
