The galaxy presents as a relatively smooth, elliptical structure with a concentrated central bulge. The core exhibits a yellowish hue, potentially indicating a population of older stars. The outer regions show a subtle blue tint, suggestive of some ongoing, albeit modest, star formation activity. There is no discernible spiral arm structure or significant dust lane presence. The galaxy's overall form appears largely undisturbed, displaying a round morphology. There may be minor signs of tidal disturbance, implying a possible past interaction, however, no significant merger activity appears to be present currently.
