The galaxy presents an elliptical morphology, appearing largely smooth and spheroidal with a high degree of central concentration. The color profile suggests a relatively evolved stellar population, trending towards redder wavelengths in the G, R, and Z bands.  Faint hints of bluer light are observed in the periphery, which are likely regions with some ongoing but weak star formation.  No distinct spiral arms or bar structures are discernible, supporting the classification of a smooth galaxy. The general appearance is relatively undisturbed, with no obvious signs of major merging events or tidal disruptions. It is moderately luminous, indicating a substantial stellar mass.
