The galaxy presents as a fairly smooth elliptical or lenticular type system. The central bulge region appears bright, exhibiting a yellowish-white color, suggesting a population of older stars. The light becomes less concentrated radially away from the core. There is a relatively small disk component. No distinct spiral arm structure is immediately apparent from the image. There are no indications of major mergers or significant tidal disturbances in the immediate vicinity of the galaxy. 
