  We present the first INTEGRAL results on Cyg X-3 from the PV phase
observations of the Cygnus region. The source was clearly detected by the
JEM-X, ISGRI and SPI detectors. The INTEGRAL observations were supported by
simultaneous pointed RXTE observations. Their lightcurves folded over the 4.8
hour binary period are compatible with the mean RXTE/ASM and CGRO/BATSE light
curves. We fit our broad band X-ray/Gamma-ray spectra with a physical model,
which represents the first such published model for Cyg X-3. The main physical
processes in the source are thermal Comptonization and Compton reflection with
parameters similar to those found for black-hole binaries at high Eddington
rates.
