The galaxy presents a largely smooth morphology, with an elliptical or lenticular shape. The central region is a bright, concentrated bulge that graduates into a somewhat less bright, diffuse halo. The overall color is skewed toward the redder end of the spectrum; some reddening may be attributed to the galaxy's inherent stellar populations. There is no evidence of spiral arms or a disk component. Additionally, there are no readily apparent signs of any ongoing major merger activity, tidal tails, or other strong gravitational disturbances. The galaxy exhibits a fairly regular, well-defined structure, suggesting it is a relatively mature system.
