The galaxy presents as a generally smooth, centrally concentrated object with a moderate degree of radial symmetry. Its overall shape appears neither perfectly spherical nor significantly elongated. The primary body of the galaxy exhibits a notable color gradient, transitioning from a bluer hue in the outer regions to a redder hue within the central core. The periphery of the galaxy appears diffuse and ill-defined. A slight asymmetry may be present in the outer regions, but no prominent features, spiral arms, or distinct disk structures are readily apparent. There is no overwhelming evidence of ongoing major merger activity. The central region shows a bright concentration, consistent with the presence of a galactic bulge.
