The galaxy presents as a disturbed morphology, strongly suggesting an ongoing or recent interaction or merger event. The main body exhibits a somewhat elongated shape, but it is difficult to describe it in a simple manner.

The object displays an irregular light distribution, with multiple bright cores. One of the cores is more yellowish, while the other has a slight red tinge to it. There is a clear tidal feature, with a bridge or arm extending outwards from the main body of the galaxy. This arm is relatively faint and shows a bluish hue. There might be evidence of disturbed dust lanes or star formation regions within the tidal arm.

The overall color of the galaxy suggests a mix of stellar populations, with evidence of both older, redder stars and younger, bluer stars, indicative of recent star formation possibly triggered by the interaction. The lack of clear spiral arm structure or a well-defined disk supports the classification of a disturbed system.
