The galaxy appears to be a relatively smooth, elliptical system. It presents with a concentrated central bulge that gradually fades outward into a diffuse halo. The color profile suggests a dominance of older stellar populations. There is little indication of spiral arms or significant dust lanes. The galaxy exhibits a slightly elongated shape. No obvious signs of active galactic nuclei activity are apparent from the image. There are no indications of ongoing major mergers or tidal disturbances.
