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Results of the CCD observations of CzeV404 Her are displayed. During theseason of June-August 2014 we detected one outburst and one superoutburst ofthe star. Clear superhumps with the period of P_sh=0.10472(2) days wereobserved. The superhump period was decreasing with a high value ofP_dot=-2.43(8) x 10^(-4). For 17 eclipses, we calculated an orbital period withthe value of P_orb=0.0980203(6) days which indicates that CzeV404 Her belongsto period gap objects and it is the longest orbital period eclipsing SU UMastar. Based on superhump and orbital period determinations, the period excess6.8 % +/- 0.02 % and the mass ratio q ~ 0.32 of the system were obtained.

CzeV404 - an eclipsing dwarf nova in the period gap during its July 2014 superoutburst