The galaxy appears as a centrally concentrated, smooth object with a largely spheroidal morphology. The color profile suggests an older stellar population, with a dominant yellow hue in the central regions indicative of evolved stars. The overall structure lacks any prominent spiral arms or disk-like features. There is some color variation towards the outer regions, potentially indicating patches of younger stars or differing metallicities, although these are not sharply defined. No signs of significant tidal disturbances or mergers are apparent, and the galaxy presents a relatively undisturbed appearance.
