The galaxy presents as an elongated structure. There appears to be a brighter, more concentrated region at one end, with a less defined, more diffuse region trailing away from it. The color gradient transitions from a yellow-white hue in the concentrated region to a bluish-white hue in the diffuse tail. There may be some degree of tidal disruption present, suggested by the elongated shape and diffuse nature of the trailing region. It is potentially undergoing a minor interaction or merger with another galaxy. The overall morphology appears to be relatively smooth.
