NGC 2617 has attracted a lot of attention after the detection of the changes in spectral type, and its geometry and kinematics of broad-line region (BLR) are still ambiguous. In this paper, we present the high cadence ($sim$ 2 days) reverberation mapping campaign of NGC 2617 from 2019 October to 2020 May undertaken at Lijiang 2.4 m telescope. For the first time, the velocity-resolved reverberation signature of the object was successfully detected. Both H$alpha$ and H$beta$ show an asymmetrical profile with a peak in the velocity-resolved time lags. For each of both lines, the lag of the line core is longer than those of the relevant wings, and the peak of the velocity-resolved lags is slightly blueshifted. These characteristics are not consistent with the theoretical prediction of the inflow, outflow or Keplerian disk model. Our observations give the time lags ofH$alpha$, H$beta$, H$gamma$, and He I, with a ratio of $tau_{rm{H}alpha}$:$tau_{rm{H}beta}$:$tau_{rm{H}gamma}$:$tau_{rm{He~I}}$ = 1.27:1.00:0.89:0.20, which indicates a stratified structure in the BLR of the object. It is the first time that the lags of H$alpha$ and He I are obtained. Assuming a virial factor of $f$ = 5.5 for dispersion width of line, the masses of black hole derived from H$alpha$ and H$beta$ are $rm{23.8^{+5.4}_{-2.7}}$ and $rm{21.1^{+3.8}_{-4.4}} times 10^{6}M_{odot}$, respectively. Our observed results indicate the complexity of the BLR of NGC 2617.
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