  Results of the CCD observations of CzeV404 Her are displayed. During the
season of June-August 2014 we detected one outburst and one superoutburst of
the star. Clear superhumps with the period of P_sh=0.10472(2) days were
observed. The superhump period was decreasing with a high value of
P_dot=-2.43(8) x 10^(-4). For 17 eclipses, we calculated an orbital period with
the value of P_orb=0.0980203(6) days which indicates that CzeV404 Her belongs
to period gap objects and it is the longest orbital period eclipsing SU UMa
star. Based on superhump and orbital period determinations, the period excess
6.8 % +/- 0.02 % and the mass ratio q ~ 0.32 of the system were obtained.
