We present a study of simultaneous determination of mean distance and reddening to the Small Magellanic Cloud ( SMC ) using the two photometric band RR Lyrae data . Currently available largest number of highly accurate and precise light curve data of the fundamental mode RR Lyrae stars ( RRab ) with better areal coverage released by the Optical Gravitational Lensing Experiment ( OGLE ) -IV project observed in the two photometric bands ( V,I ) were utilised simultaneously in order to determine true distance and reddening independently for each of the individual RRab stars . Different empirical and theoretical calibrations leading to the determination of absolute magnitudes of RRab stars in the two bands , V and I along with their mean magnitudes were utilised to calculate the apparent distance moduli of each of these RRab stars in these two bands . Decomposing the apparent distance moduli into true distance modulus and reddening in each of these two bands , individual RRab distance and reddening were estimated solving the two apparent distance moduli equations . Modeling the observed distributions of the true distance moduli and reddenings of the SMC RRab stars as Gaussian , the true mean distance modulus and mean reddening value to the SMC were found to be \mu _ { 0 } = 18.909 \pm 0.148 mag and E ( B - V ) = 0.066 \pm 0.036 mag , respectively . This corresponds to a distance of D = 60.506 \pm 4.126 kpc to the SMC . The three dimensional distribution of the SMC RRab stars was approximated as ellipsoid . Then using the principal axes transformation method \citep deb14 we find the axes ratios of the SMC : 1.000 \pm 0.001 , 1.113 \pm 0.002 , 2.986 \pm 0.023 with i = 3 ^ { \circ } .156 \pm 0 ^ { \circ } .188 and \theta _ { \text { lon } } = 38 ^ { \circ } .027 \pm 0.577 . These results are in agreement with other recent independent previous studies using different tracers and methodologies .