  The structure of our Galaxy has been studied from ultraviolet (UV) star
counts obtained with the Ultra-Violet Imaging Telescope (UVIT) on board the
{\em AstroSat} satellite, in Far-UV (FUV) and Near-UV (NUV) bands. The F154W
(BaF2) and N263M (NUVB4) filters were used in the FUV and NUV bands,
respectively. The point sources are separated from the extra-galactic sources
of UVIT observations using infrared (IR) color cut method. The observed UVIT
star counts match well with the simulations obtained from the Besan\c{c}on
model of stellar population synthesis towards several Galactic directions. We
also estimated the scale length and scale height of the thick disc and the
scale height of the thin disc using the space density function and the
exponential density law for the stars of intermediate Galactic latitudes. The
scale length of the thick disc ranges from 3.11 to 5.40 kpc whereas the scale
height ranges from 530$\pm$32 pc to 630$\pm$29 pc. The scale height of the thin
disc comes out to be in the range of 230$\pm$20 pc to 330$\pm$11 pc.
