The galaxy presents a spiral morphology with a prominent disk. The spiral arms appear loosely wound, tracing a somewhat irregular pattern throughout the disk. The galaxy's light distribution suggests a central bulge is present, though not particularly dominant. A bar structure is potentially present, but the evidence is not conclusive from this image. The disk is not viewed perfectly face-on, but is seen at an angle. There appears to be at least one other galaxy interacting with the spiral, which has caused disturbances to the spiral arms.
