The galaxy presents as a somewhat elliptical, centrally concentrated object. The light distribution appears mostly smooth with a hint of some disturbances. The core region exhibits a concentration of luminosity. The object shows a gradient in color, with the central region appearing more yellow-orange, suggesting a population of older stars. The outer regions appear slightly bluer suggesting some ongoing star formation. There may be evidence of some minor disturbance in the morphology, possibly indicating an interaction or recent merger event. The galaxy does not appear to be a classical spiral or a well-defined elliptical galaxy.
