  New results from long-term optical photometric observations of the pre-main
sequence star GM Cep from UX Orionis type are reported. During ongoing
photometric monitoring of the GM Cep four deep minimums in brightness are
observed. The collected multicolour photometric data shows the typical of UXor
variables colour reversal during the minimums in brightness. Recent $BVRI$
photometric observations of GM Cep have been collected from November 2014 to
October 2020.
