The galaxy appears to be a relatively smooth, centrally concentrated system. It exhibits a generally elliptical morphology with a dominant, bulge-like structure. The color profile suggests a population of older stars, inferred from the yellow/orange hue that is more prominent within the central regions. Fainter, somewhat bluer regions are observed in the outskirts. There is no strong evidence of spiral arm structure or significant dust lanes. There may be a slight tidal disturbance to the galaxy, however it looks as though this is a relatively undisturbed system overall.
