The galaxy presents as a centrally concentrated object with a smooth, spheroidal morphology. There is a discernible color gradient, with a yellowish-white core gradually fading into a bluish halo. No distinct spiral arms or other fine structures are visible. The galaxy appears relatively isolated, exhibiting no obvious signs of tidal interactions or major disturbances that could indicate a recent merger event, although there might be some minor disturbances. Its overall roundness suggests a classification leaning towards elliptical or lenticular. The color profile implies a moderate level of star formation activity, though it is unlikely to be extremely active given the overall smoothness and lack of pronounced features.
