The galaxy appears as a centrally concentrated object with a largely smooth, elliptical morphology. The core region is a bright, yellowish-white hue, suggesting an older stellar population. Fainter light extends outward from the central region in a more diffuse and reddish gradient. There is no discernible spiral arm structure nor any apparent ongoing merger or major disturbances. The galaxy is a fairly isolated and relaxed system with signs of some past star formation.
