The galaxy presents as a relatively smooth, centrally concentrated object. There is no indication of spiral arm structure or a pronounced disk; the light profile appears generally elliptical or spheroidal. The central region is bright and appears somewhat yellowish, possibly indicating an older stellar population or dust obscuration. The overall color of the galaxy seems to be more weighted toward the redder part of the spectrum. The galaxy exhibits a fairly regular shape, displaying a degree of roundness. There are no obvious signs of major ongoing mergers or significant tidal disturbances affecting its morphology. The system displays a seemingly minimal degree of current star formation.
