The galaxy presents as a single, concentrated object with a smooth morphology. It exhibits an elliptical shape with a high degree of roundness. Light distribution is centrally concentrated, appearing brightest in the core region, with a gradual decrease in luminosity toward the outer edges. There is no apparent spiral arm structure or disk. No signs of recent or ongoing mergers or major disturbances are visible; the galaxy appears relatively isolated and undisturbed. Overall color is a yellowish-white, suggesting an older stellar population.
