The galaxy appears as a somewhat irregular, disk-shaped structure. There is evidence of tidal disturbances, potentially indicating a past or ongoing merger event. The central region presents a moderate bulge, which is not overly dominant. There are not distinct spiral arms, although there seems to be some form of ordered structure within the disk. The object has a blueish hue, especially towards the disk, which suggest the presence of ongoing star formation. It is not seen as an edge-on system. 
