The galaxy presents as a largely featureless elliptical. It exhibits a smooth, centrally concentrated light profile, with a notable lack of spiral arms or a distinct disk component. The morphology appears consistently rounded. Color gradients suggest a slightly redder core transitioning to a marginally bluer halo region. There are no apparent signs of ongoing major mergers or tidal disturbances in the immediate vicinity. The overall appearance indicates a relatively evolved stellar population with minimal recent star formation activity.
