  Results from BVRI photometric observations of the pre-main sequence star
V1704 Cyg collected during the time period from August 2010 to December 2017
are presented. The star is located in the star-forming HII region IC 5070 and
it exhibits photometric variability in all-optical passbands. After analyzing
the obtained data, V1704 Cyg is classified as a classical T Tauri star.
