The galaxy presents as a centrally concentrated object with a smooth, relatively featureless appearance. The light profile suggests a spheroidal morphology, likely an elliptical galaxy or a lenticular galaxy viewed face-on. There's no evidence of spiral arms or a distinct disk structure visible in this image. The core exhibits a bright, yellowish-white hue, potentially indicating a population of older stars. Moving outwards from the core, the color gradually shifts towards a redder tone, which might be related to a change in stellar population or dust content at the outskirts. The overall shape appears generally round with a slight ellipticity, and shows no signs of major tidal distortions or ongoing mergers. Subtle color variations within the galaxy body are also present, likely reflecting localized differences in star formation rates or metallicity.
