The galaxy presents a largely smooth and rounded morphology. Its light profile suggests an elliptical structure, with a concentration of older stellar populations. No distinct spiral arms or prominent features like dust lanes are visible. A slight yellow tint indicates a dearth of recent star formation and a high concentration of evolved stars. The overall appearance suggests the galaxy is relatively undisturbed, showing no significant signs of ongoing or recent merger activity. The galaxy has a relatively compact apparent size, inferring a considerable distance.
