[en] Using observations of the INTErnational Gamma-Ray Astrophysics Laboratory (INTEGRAL), we place upper limits on the gamma-ray and hard X-ray prompt emission associated with the gravitational wave event GW150914, which was discovered by the LIGO/Virgo Collaboration. The omnidirectional view of the INTEGRAL/SPI-ACS has allowed us to constrain the fraction of energy emitted in the hard X-ray electromagnetic component for the full high-probability sky region of LIGO triggers. Our upper limits on the hard X-ray fluence at the time of the event range from $F_{\mathrm{\gamma <!--\; ??\; -->}}=2\times <!--\; ??\; -->{10}^{-<!--\; ???\; -->8}$ erg cm⁻² to $F_{\mathrm{\gamma <!--\; ??\; -->}}={10}^{-<!--\; ???\; -->6}$ erg cm⁻² in the 75 keV–2 MeV energy range for typical spectral models. Our results constrain the ratio of the energy promptly released in gamma-rays in the direction of the observer to the gravitational wave energy E ${}_{\mathrm{\gamma <!--\; ??\; -->}}/$ E ${}_{\mathrm{G}\mathrm{W}}<<!--\; <\; -->{10}^{-<!--\; ???\; -->6}$. We discuss the implication of gamma-ray limits for the characteristics of the gravitational wave source, based on the available predictions for prompt electromagnetic emission.