Polycyclic aromatic hydrocarbons are considered as primary carriers of the unidentified interstellar bands. The recent discovery of the first interstellar aromatic molecule, benzonitrile (C 6 H 5 CN), suggests a repository of aromatic hydrocarbons in the outer earth environment. Herein, we report an infrared (IR) study of benzonitrile−(D 2 O) n clusters using mass-selective detection in helium nanodroplets. In this work, we use isotopically substituted water, D 2 O, instead of H 2 O because of our restricted IR frequency range (2565−3100 cm −1 ). A comparison of the experimental and predicted spectra computed at the MP2/6-311++G(d,p) level of benzonitrile−(water) 1−2 clusters reveals the formation of a unique local minimum structure, which was not detected in previous gasphase molecular beam experiments. Here, the solvent water forms a nearly linear hydrogen bond (H-bond) with the nitrile nitrogen of benzonitrile, while the previously reported most stable cyclic H-bonded isomer is not observed. This can be rationalized by the stepwise aggregation process of precooled monomers. The addition of a second water molecule results in the formation of two different isomers. In one of the observed isomers, a H-bonded water chain binds linearly to the nitrile nitrogen similar to the monohydrated benzonitrile−water complex. In the other observed isomer, the water dimer forms a ring-type structure, where a H-bonded water dimer simultaneously interacts with the nitrile nitrogen and the adjacent ortho CH group. Finally, we compare the water-binding motif in the neutral benzonitrile−water complex with the corresponding positively and negatively charged benzonitrile−water monohydrates to comprehend the charge-induced alteration of the solvent binding motif.