 The star has been found to display deep, irregularly shaped transits suggestive of disrupted planetary debris.Two transits have been observed in the 210-day-long Zwicky Transient Facility (ZTF) light curve of the star, each transit about 25 days long and producing 30−45% dips in brightness.The two transits are about 110 days apart, substantially longer than the short 4.5 hour orbital period seen with WD1145+017.