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New photometric data from CCD UBVRI observations of the PMS star V350 Cepduring the period from March 2014 to May 2017 are presented. In the periodApril-May 2016 we registered a deep fades event in the brightness of the starwith amplitudes $\Delta I$ = 1.75 mag, $\Delta R$ = 1.69 mag, $\Delta V$ = 1.77mag and $\Delta B$ = 2.16 mag. Simultaneously with the fades in the brightness,the change in the star's color indices has been observed. V350 Cep indicatesthe typical for stars of UXor type "blueing effect" during the deep minimum ofbrightness. During the second half of 2016 V350 Cep restores its brightness toa level close to the maximum. Since the star has been studied as a possibleFUor object in previous studies, the possible cause of the deep decline is adecrease in the accretion rate. Another possible cause is obscuration fromclumps of dust orbiting at the vicinity of the star.

A deep decrease event in the brightness of the PMS star V350 Cep