The galaxy presents a largely smooth morphology, exhibiting a centrally concentrated structure with a high degree of circular symmetry. There is minimal evidence of significant disk features or spiral arms. A bright, condensed core is evident. A diffuse, extended halo surrounds the core, gradually fading into the background. Subtle color variations are visible within the halo. The galaxy's overall appearance suggests a relatively evolved system, potentially an elliptical galaxy or a lenticular galaxy seen at a significant distance. There are only slight signs of disturbance, suggesting that this galaxy has not undergone any recent mergers.
