The galaxy presents as a spiral type, although some characteristics point to an irregular morphology. It has a discernible disk, and is not seen edge-on. There are indications of spiral arm structure, with a blue hue, suggesting recent star formation. A bar structure also seems present, but difficult to distinguish. There is a noticeable bulge, somewhere between a moderate or small size, suggesting that the galaxy is not a late-type spiral. Furthermore, signs of ongoing or recent merger activity are present, including a disturbed morphology and an asymmetrical light distribution. Overall, the galaxy appears to be actively evolving.
