The galaxy presents as a relatively smooth, centrally concentrated object with an elliptical morphology. Its color profile suggests an older stellar population, with a yellowish hue dominating the central region. There is little evidence of significant spiral arm structure or dust lanes. The outer regions exhibit a gradual decrease in surface brightness, indicating a diffuse halo. Minor asymmetry is observed along one edge, potentially indicative of a minor tidal interaction or disturbance, but it does not suggest a major ongoing merger event. Overall, the galaxy appears to be a relatively evolved system with a high degree of central symmetry and low levels of current star formation.
