The galaxy appears to be a relatively smooth, elliptical-like structure. It exhibits a concentrated central bulge that emits strongly in yellow-orange wavelengths, possibly indicating an older stellar population. There is little evidence of prominent spiral arms or significant dust lanes. The overall shape of the galaxy is quite round. There is a subtle extension of light surrounding the core, indicating the presence of a more diffuse halo. There are no obvious signs of any ongoing major mergers or significant tidal disturbances. The galaxy is not perfectly spherical but rather a soft round shape.
