The galaxy presents a largely smooth, elliptical morphology. Its overall structure appears rounded, with a high degree of radial symmetry. The central region exhibits a bright, concentrated core. There is no clear evidence of spiral arms or a prominent disk structure. Color gradients suggest a potential variation in stellar populations, with the central region appearing more yellow, indicative of older stars, and the outer regions displaying bluer hues. There are no obvious signs of major ongoing merger events, though subtle irregularities in the outer regions suggest a possibility of minor interactions or disturbances. The relatively smooth appearance points towards a lack of significant recent star formation.
