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\rm Observations of close binary system (CBS) V1357 Cyg=Cyg X-1 in the $WBVR$bands are reported. Photometry was carried out at the telescopes located inKazakhstan, Uzbekistan and Crimea equipped with single-channel$WBVR$-photometer with photon counting. 1358 individual observations in $WBVR$bands on 202 nights were obtained.  The analysis of the photometric data allows to conclude that differentphotometric effects are superimposed on the orbital light curve of the system.Among them are brightness declines, outbursts with different duration andamplitude, chaotic variability, which sometimes exceeded the ellipsoidalvariability. Strong brightness decreases with magnitude $0^m.035 - 0^m.045$ areobserved, they are equal to the contribution of accretion disc to the totalluminosity of the system.  10 years of photometric monitoring allowed to detect continous brightening ofthe system, followed by luminosity decline (slow outburst). After the maximumin 1994-96 the decline was equal to 7% in the $W$ band, 4% in the $V$ band, and2% in the $V$ and $R$ bands.  This paper continues the series of works on close systems with X-ray sources.  \textbf{Key words}: Close binary systems - luminosity - ellipsoidalvariability - accretion disc

Multicolor electrophotometry of the peculiar object V1357 Cyg=Cyg X-1 in the period 1986 -- 1992