The galaxy presents a primarily smooth, elliptical morphology. The light distribution indicates a concentration of older stellar populations towards the center, exhibiting a yellowish hue. Fainter and more diffuse bluer light is present in what appears to be the outer regions of the galaxy. The galaxy has a fairly high degree of symmetry, although it appears slightly elongated. A faint irregular feature is present along the outside of the galaxy. There is no apparent spiral structure. Based on the color gradients and overall light distribution, star formation may be ongoing at a low rate.
