The galaxy presents a largely smooth, elliptical morphology. The primary body exhibits a concentrated, round structure with a yellowish hue, suggesting an older stellar population and a diminished rate of active star formation. Subtle color gradients appear, with the core region being more intensely yellow, possibly indicating a higher density of older stars or dust obscuration. The outer regions show a faint blue tinge, implying the presence of a younger, though still relatively quiescent, stellar population. There is no obvious sign of a spiral arm structure. The overall appearance is consistent with an evolved galaxy residing at a considerable distance, exhibiting no major signs of recent merging events.
