With the ever growing global population, demand for new abundant sources of energy is on the rise. Solar power is one such source, and despite technology dating back several decades, it has failed to gain major traction due to both the cost of materials and processing of silicon semiconductors, which currently dominate the market. One promising replacement for silicon is copper tin zinc sulfide (CZTS), and its selenated derivatives, CZTSSe, and CZTSe. The bandgap of these materials is adjustable by varying the ratio of sulfur and selenium, S/(S+Se), and lies between 1.0 and 1.5 eV, an ideal range for photovolatics (PV). CZTS solar cells consist of earth abundant materials which are inexpensive to process. One such method, the molecular precursor route, involves making solutions of the precursor materials, including copper (I), zinc (II), tin (IV), thiourea (tu) as a sulfur source, and dimethyl sulfoxide (DMSO). Once the solution forms, thin films are spin coated onto molybdenum (Mo) coated substrate and thermally annealed at 500°C to form the CZTS crystal structure and absorber layer before subsequent processing steps. In this solution, metal-thiourea, metal-DMSO and metal-thiourea-DMSO complexes of various geometries and constitution are formed. Using density functional theory (DFT), the stability of these complexes has been probed to determine their relative stability in order to understand the contents of the solution and to optimize the precursor solution to improve the efficiency of CZTS. By choosing precursor chemicals which form complexes of varying stability, the CZTS molecular ink formulation can be modified and CZTS absorber material quality can be improved. Complexes such as Zn(DMSO)2Cl2, Zn(tu)2Cl2, and Sn(DMSO)6 have been investigated using DFT calculation methods within Gaussian. Both the vacuum and solvated energies have been investigated and compared to gain insight into what complexes are present in the molecular precursor solution.