  We present results of spectral analysis of Ginga data obtained during the decline phase after the 1989 outburst of GS 2023+338 (V404 Cyg). Our analysis includes detailed modelling of the effects of X-ray reflection/reprocessing. We have found that   (1) the contribution of the reprocessed component (both continuum and line) corresponds to the solid angle of the reprocessor as seen from the X-ray source of Omega \approx (0.4-0.5) 2\pi,   (2) the reprocessed component (both line and continuum) is broadened (``smeared'') by kinematic and relativistic effects, as expected from the accretion disk reflection.   We discuss the constraints these results give on various possible system geometries. 
Relativistically smeared X-ray reprocessed components in the GINGA   spectra of GS 2023+338