Analysis of a new variable star CzeV753 in Cygnus is presented. It was discovered during observation of an RR Lyrae star V1949 Cyg in 2015. Based on the shape of the light curve and its characteristics (period of 0.387162 d, amplitude of 0.313 mag), the new variable star is an eclipsing binary of W Ursae Majoris type. According to the B-V=0.344 mag from literature the CzeV753 is probably an F-type star.