The galaxy presents as an elliptical morphology with a high degree of central concentration. Its overall color profile suggests an older stellar population, dominated by redder wavelengths, with minimal presence of bluer, younger stars. The galaxy exhibits a smooth texture and a generally undisturbed appearance; there are no discernible tidal features, plumes, or other signs of recent or ongoing major mergers. The galaxy appears quite round. There is a potential for minor asymmetry or subtle disturbance, which could indicate minor interaction history or internal processes such as bar formation, although these features are not strongly pronounced. The object's magnitude suggests it is a fairly luminous galaxy, despite its distance, exhibiting high mass. Overall, it appears to be a massive elliptical galaxy that is undergoing only a small amount of star formation.