GK Per is a unique cataclysmic variable star which has showed a nova explosion as well as dwarf novatype outbursts, and has the intermediate-polar nature. We carried out V -band time-resolved photometry and B-band monitoring during the 1996 outburst. This outburst lasted about 60 d and is divided into three parts: the slow rise branch for 35 d, the gradual decay branch with a decay rate of 20.0 d mag −1 for ∼16 d, and the rapid decline branch with a rate of 5.6 d mag −1 for ∼10 d. The B − V color became bluest (B − V ∼ 0.18) about 10 d before the outburst maximum, which supports an idea that the outburst in GK Per is of the inside-out type. The spin pulse, 440-s quasi periodic oscillations (QPOs), and ∼5,000-s QPOs were detected in our light curve, as previously seen in X-ray and optical observations. In addition, we report the discovery of ∼300-s periodicity, which is shorter than the spin period.