The galaxy appears to be a relatively smooth, elliptical system. It exhibits a concentrated central bulge that graduates smoothly into a more diffuse halo. The core region has a yellow-white color, suggestive of an older stellar population. No distinct spiral arms or significant dust lanes are discernible in this image. There is a very subtle color gradient as you move outwards from the core to the edge of the halo. Overall, the galaxy appears as an isolated system showing no strong signs of tidal interactions or mergers.
