The galaxy appears as a centrally concentrated object with an elliptical morphology. It exhibits a smooth light distribution, lacking any apparent spiral arms or distinct features. The color profile suggests a relatively evolved stellar population, with a subtle reddish hue dominating the central region, potentially indicative of older stars. The outer regions appear slightly bluer, hinting at possible ongoing, but subdued, star formation. There is no obvious evidence of a major merger or significant tidal disturbances, though a minor asymmetry or subtle distortion cannot be entirely ruled out. The galaxy's apparent elongation indicates a non-spherical shape, likely an oblate spheroid. Overall, this galaxy appears to be a relatively undisturbed elliptical galaxy with modest levels of star formation.
