The galaxy presents as a luminous, elliptical object. Its light profile appears smooth and centrally concentrated, with a gradual decrease in intensity outwards from the core. The color is generally yellow-white, suggesting an older stellar population. There may be a small population of younger stars, as faintly indicated by some green-blue hues. No distinct spiral arm structures or significant dust lanes are discernible. The overall morphology suggests a galaxy that has largely completed its major star formation epoch, indicating a quiescent or passively evolving system.
