The galaxy appears as a roughly circular, unresolved object. The light profile indicates a relatively smooth distribution, with a centrally concentrated core region that transitions outwards to a more diffuse halo. The core exhibits a yellowish-white hue, potentially indicative of an older stellar population dominating this region. Moving away from the center, the halo appears slightly redder and fainter. The overall morphology suggests a high degree of symmetry and a lack of pronounced spiral arms or other distinct structural features. There is no obvious dust lane. It's possible that this galaxy is an elliptical, or perhaps a lenticular galaxy, but it would take more resolved observations to find out for sure. There are no indications of a major ongoing merger, although there may be subtle distortions that hint at a minor interaction in its past.
