The galaxy presents as a largely featureless elliptical or lenticular morphology. It exhibits a smooth, concentrated light profile, with a high degree of central brightness and radial symmetry. The core region presents a yellow-orange hue, suggesting a population of older stars and a reduced rate of on-going star formation, which dims into a redder halo. There's no visible spiral arm structure or prominent dust lanes. There might be some slight disturbances but generally shows no strong evidence of recent major merger activity, although minor interactions cannot be ruled out. The roundness of the galaxy suggests a more face-on orientation relative to our line of sight. Overall, the galaxy appears to be a relatively evolved system with characteristics consistent with those of a massive galaxy.
