The galaxy presents a generally smooth, elliptical morphology. The light profile is centrally concentrated with a gradual decline in intensity outward from the core. There are no readily apparent spiral arms or dust lanes. The overall color is consistent with an older stellar population, appearing slightly redder than bluer. While there are no strong signs of an ongoing merger, there are some subtle indications of minor tidal disturbances, seen as very faint extensions or asymmetries in the outer regions of the galaxy. The central region exhibits a high degree of circularity.
