The galaxy presents as a centrally concentrated, smooth object. Its morphology appears largely spheroidal, with a gradual decrease in luminosity from the core outwards. There is a slight elongation, but it's nearly round. The color profile suggests a dominant population of older stars with less active star formation. Its appearance suggests a relatively undisturbed system. The galaxy shows a redder color. No dust lanes or prominent spiral structures are apparent. Overall, the galaxy appears to be a relatively massive, passively evolving system.
