The galaxy presents a largely smooth, elliptical morphology. A bright, concentrated central bulge dominates the core, fading into a more diffuse, less structured halo. The overall color appears to be somewhat blue, which could mean that there are populations of younger stars in the galaxy. There is no apparent dust lane or any signs of spiral arm structure. The galaxy is mostly rounded but there may be some evidence of it being slightly more of an in-between shape. There are no obvious signs of any ongoing major mergers or significant tidal disturbances. 
