The galaxy appears as a relatively smooth, centrally concentrated object. Its overall shape is somewhat rounded. There may be a very subtle disk structure, but the image resolution limits conclusive identification. Color gradients suggest a possible older stellar population dominating the central regions. The galaxy appears relatively undisturbed, lacking any obvious signs of major mergers or significant tidal interactions. A faint, diffuse halo extends beyond the main body of the galaxy. The galaxy's integrated color indicates moderate levels of star formation.
