The galaxy presents as a smooth, centrally concentrated object with an elliptical morphology. A bright, condensed nucleus dominates the central region, surrounded by a diffuse halo of light that extends outwards, fading gradually into the background. The color profile suggests a generally older stellar population, with a slight bluer tint compared to the redder color expected of elliptical galaxies, indicating some presence of younger stars or on-going star formation. There is no apparent spiral structure or strong dust lanes. The overall appearance indicates a galaxy that is likely a relatively quiescent system. Close inspection reveals no signs of major mergers or significant tidal disturbances. The galaxy is not perfectly spherical.
