The photographic magnitudes mpg, mpv, mpr of the Fuor V1057 Cygni for July 1968 - August 1970 and photoelectric UBVRI' observations made in July 1978 - December 1985 are presented. In the epoch of light increase and light maximum 26 estimations of mpg, 20 mpv and 3 mpr for V1057 Cygni have been obtained. The upper limit of the color-index V-1 < 3m.5 in the preoutburst epoch is estimated. A periodic component with the period of about 12 days and amplitude of about 0m.1 V was derived from the light curves in B, V, R for 300 observational nights. From 1982 to 1986 the rate of brightness decrease did not exceed 0m.2 V while during four previous years the light decrease was ∆V > 0m.4.
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