The galaxy presents as a relatively smooth, centrally concentrated object, appearing largely featureless. The core exhibits a bright, yellowish-white hue, suggesting a significant population of older stars. This core region transitions outwards to a more diffuse, reddish halo, implying the presence of a lower-density stellar population or dust. The overall morphology suggests an elliptical or lenticular galaxy, showing little evidence of spiral arms or active star formation. There is no visible indication of any major merger events or significant tidal disturbances affecting the system.
