The galaxy presents as a centrally concentrated, elliptical-like structure, exhibiting a high degree of smoothness. It is highly symmetric, with a gradual decrease in luminosity from the core. The color gradient shows a yellowish-gold central region, possibly indicative of an older stellar population, transitioning to a redder outer halo. There is no visual evidence of spiral arms or significant dust lanes. Faint irregularities may be present in the outermost regions, suggestive of minor interactions or past mergers, however, this is unconfirmed. The galaxy appears largely undisturbed. Overall, it is a mature system with minimal ongoing star formation.
