The galaxy appears as a somewhat diffuse, relatively small object. There is low overall surface brightness. It is not strongly centrally concentrated. The object shows signs of significant disruption, with an irregular morphology. There may be some evidence of tidal features or extended structure suggesting a possible recent or ongoing merger event, with a lumpy shape. There is at least one noticeable region within the galaxy where star formation appears more active, as evidenced by its slightly brighter emission.
