We developed a spectroscopic monitoring project to investigate the kinematics of the broad-line region ( BLR ) in active galactic nuclei ( AGN ) with ultra-fast outflows ( UFOs ) . Mrk 79 is a radio-quiet AGN with UFOs and warm absorbers , had been monitored by three reverberation mapping ( RM ) campaigns , but its BLR kinematics is not understood yet . In this paper , we report the results from a new RM-campaign of Mrk 79 , which was undertaken by Lijiang 2.4-m telescope . Mrk 79 is seeming to come out the faint state , the mean flux approximates a magnitude fainter than historical record . We successfully measured the lags of the broad emission lines including H \beta~ { } \lambda 4861 , H \gamma~ { } \lambda 4340 , He ii \lambda 4686 and He i \lambda 5876 with respect to the varying AGN continuum . Based on the broad H \beta~ { } \lambda 4861 line , we measured black hole ( BH ) mass of M _ { \bullet } = 5.13 ^ { +1.57 } _ { -1.55 } \times 10 ^ { 7 } M _ { \odot } , estimated accretion rates of { \dot { M } _ { \bullet } } = ( 0.05 \pm 0.02 ) ~ { } L _ { Edd } ~ { } c ^ { -2 } , indicating that Mrk 79 is a sub-Eddington accretor . We found that Mrk 79 deviates from the canonical Radius - Luminosity relationship . The marginal blueshift of the broad He ii \lambda 4686 line detected from rms spectrum indicates outflow of high-ionization gas . The velocity-resolved lag profiles of the broad H \gamma~ { } \lambda 4340 , H \beta~ { } \lambda 4861 , and He i \lambda 5876 lines show similar signatures that the largest lag occurs in the red wing of the lines then the lag decreases to both sides . These signatures should suggest that the BLR of Keplerian motion probably exists the outflow gas motion . All findings including UFOs , warm absorbers , and the kinematics of high- and low-ionization BLR , may provide an indirect evidence that the BLR of Mrk 79 probably originates from disk wind .