The galaxy presents as an elliptical shape. There appears to be a bright central bulge, with a moderate concentration of light. The outer regions of the galaxy fade gradually away from the center, suggesting a smooth transition in stellar density. There is evidence of some disk-like structure, but it is not well defined. The color is generally uniform, with a slight redder hue towards the center which is indicative of an older stellar population. Fainter, bluer regions are seen in the outer edges of the galaxy, which may indicate some recent star formation. The general smoothness of the light distribution suggests the galaxy has not undergone a recent major merger event.