The galaxy presents as a predominantly smooth, elliptical structure with a bright, concentrated core. The overall color profile suggests a moderate presence of older stellar populations, indicated by the yellowish-white hue concentrated centrally. The galaxy exhibits a slight elongation, with an apparent axis ratio suggesting it is not perfectly spherical. Some subtle dust lanes or faint spiral arm segments may be present, but these features are not sharply defined, indicating a system without substantial ongoing, high-rate star formation. A very minor disturbance can be seen on the far left of the galaxy. The radial color gradient suggests a gradual decline in older stellar populations outwards from the center.
