Cu 2 ZnGeSe 4 is of interest for the development of next-generation thin-film photovoltaic technologies. To understand its electronic structure and related fundamental optical properties, we performed first-principles calculations for three structural variations: kesterite, stannite, and primitive-mixed CuAu phases. The calculated data are compared with the room-temperature dielectric function ε = ε 1 + iε 2 spectrum of polycrystalline Cu 2 ZnGeSe 4 determined by vacuumultraviolet spectroscopic ellipsometry in the photon-energy range of 0.7 to 9.0 eV. Ellipsometric data are modeled with the sum of eight Tauc-Lorentz oscillators, and the best-fit model yields the bandgap and Tauc-gap energies of 1.25 and 1.19 eV, respectively. A comparison of overall peak shapes and relative intensities between experimental spectra and the calculated ε data for three structural variations suggests that the sample may not have a pure (ordered) kesterite phase. The complex refractive index N = n + ik, normal-incidence reflectivity R, and absorption coefficients α are calculated from the modeled ε spectrum, which are also compared with those of Cu 2 ZnSnSe 4. The spectral features for Cu 2 ZnGeSe 4 appear to be weaker and broader than those for Cu 2 ZnSnSe 4 , which is possibly due to more structural imperfections presented in Cu 2 ZnGeSe 4 than Cu 2 ZnSnSe 4 .