The galaxy presents as a diffuse, roughly elliptical object. The central region appears slightly brighter than the outer regions. There is a subtle hint of disk-like structure, although the overall appearance is dominated by a more amorphous halo. Faint tidal features or minor disturbances cannot be ruled out upon closer inspection. The galaxy appears to have a notable amount of older stellar populations, which gives it its general color. There is evidence of low levels of star formation in certain areas, indicating that the galaxy is not completely quiescent. Analysis of the image suggest it is not currently undergoing a major merger.