The galaxy appears as a centrally concentrated, elliptical-like object. Its overall color profile suggests a relatively older stellar population, indicated by the yellowish hue of the core. There is a lack of discernible spiral arm structure or distinct dust lanes. The light is smooth with no major disturbances. It is relatively round in shape. The light suggests that star formation activity is currently low within the galaxy, which is consistent with the aged stellar population. The galaxy is a faint object, implying a considerable distance.
