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UBVRI photometry of the classical slow nova V2659 Cyg (Nova Cygni 2014), obtained with the 0.18 – 1.0m telescopes and 6/18 cm photo lense at Stará Lesná Observatory (Slovakia), Nauchny and Mt. Koshka Observatories (Russia) and Main Astronomical Observatory , Goloseevo (Ukraine), is presented. V and B light curves were used to find the basic parameters of the nova: the rate of decline, absolute magnitude at maximum, interstellar extinction and distance. Brightness variability and colour diagrams of the nova are discussed.