Clarifying the interplay between charge density waves (CDWs) and superconductivity is important in the kagome metal CsVSb, and pressure () can play a crucial role. Here, we present Sb nuclear quadrupole resonance (NQR) measurements under hydrostatic pressures up to 2.43 GPa in CsVSb single crystals. We demonstrate that the CDW gradually changes from a commensurate modulation with a star-of-David (SoD) pattern to an incommensurate one with a superimposed SoD and Tri-hexagonal (TrH) pattern stacking along the -axis. Moreover, the linewidth of Sb-NQR spectra increases with cooling down to , indicating the appearance of a short-range CDW order due to CDW fluctuations pinned by quenched disorders. The shows a Curie-Weiss temperature dependence and tends to diverge at 1.9 GPa, suggesting that a CDW quantum critical point (QCP) exists at where shows the maximum. For , spin fluctuations are enhanced when the CDW is suppressed. Our results suggest that the maximal at 1.9 GPa is related to the CDW QCP and the presence of spin fluctuations prevent the from a rapid decrease otherwise after the CDW is completely suppressed.

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