The galaxy presents an overall elliptical morphology, appearing relatively smooth in texture. There is a central bulge region with a high concentration of light, suggesting a concentration of older stars. The galaxy exhibits a gradual decline in luminosity from the core outwards. There is evidence of potential tidal disturbances, but the galaxy is otherwise well formed, not undergoing any violent mergers. There is a bluer halo around it, indicating the presence of younger stars and star formation. 
