The galaxy presents as a centrally concentrated system with a smooth, diffuse morphology. The core region exhibits a bright, nearly uniform luminosity profile suggestive of an older stellar population. There is an apparent, faint flattened disk surrounding the core, that shows possible signs of some features. It is relatively uniform in color, but there appears to be hints of spiral arms or other disk structures embedded within it. The disk appears elongated, but not particularly disturbed, with no obvious signs of tidal tails or interacting companions. The overall color indices suggest a relatively passive system with modest star formation.
