The galaxy presents as a relatively smooth, centrally concentrated object. Its morphology appears largely elliptical, with minimal discernible spiral structure or distinct features. The light profile suggests a high degree of symmetry and a centrally dominant bulge component. The color gradient indicates that it is bluer in the center and redder at its outskirts. Its light is dominated by older stellar populations, exhibiting colors consistent with evolved stars. There are no apparent signs of ongoing major mergers or significant tidal disturbances.
