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We present a deep far and near-ultraviolet (FUV and NUV) wide-field imagingsurvey of galaxies in the Bootes Void using Ultra-Violet Imaging Telescopeonboard {\em AstroSat}. Our data reach $5\sigma$ limiting magnitudes for pointsources at 23.0 and 24.0 AB mag in FUV and NUV respectively. We report a totalof six star-forming galaxies residing in the Bootes Void alongside the fullcatalog, and of these, three are newly detected in our FUV observation.  Our void galaxy sample spans a range of UV colors $(-0.35\, \leq$ FUV$-$NUV$\leq\, 0.68)$ and absolute magnitudes $(-14.16\, \leq\, \mathrm{M_{NUV}}\,\leq\, -18.65)$. In addition, {\em Sloan Digital Sky Survey} and {\emTwo-micron All Sky Survey} archival data are being used to study UV, optical,and infrared color-magnitude relations for our galaxies in the void. Weinvestigate the nature of bi-modal color distribution, morphologies, and starformation of the void galaxies. Most of the galaxies in our sample are fainterand less massive than L$^{\ast}$ galaxies, with M$_\mathrm{r} > -20$. Ouranalysis reveals a dominant fraction of bluer galaxies over the red ones in thevoid region probed. The internal and Galactic extinction corrected FUV starformation rates (SFRs) in our void galaxy catalog varies in a large range of$0.05$ to $51.01$ M$_{\odot} yr^{-1}$, with a median $3.96$ M$_{\odot}yr^{-1}$. We find a weak effect of the environment on the SFRs of galaxies.Implications of our findings are discussed.

The Ultraviolet Deep Imaging Survey of Galaxies in the Bootes Void I: catalog, color-magnitude relations and star formation