  Results from UBVRI optical photometric observations of the pre-main sequence
star V350 Cep during the period 2004-2014 are presented. The star was
discovered in 1977 due to its remarkable increase in brightness by more than 5
mag (R). In previous studies, V350 Cep was considered a to be a potential FUor
or EXor eruptive variables. Our data suggest that during the period of
observations the star maintains its maximum brightness with low amplitude
photometric variations. Our conclusion is that V350 Cep was probably an
intermediate object between FUors and EXors, similar to V1647 Ori.
