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The masses and radii determined for the components are $M_1$ =0.870$\\pm$0.074\\Msun, $M_2$=0.607$\\pm$0.053\\Msun and $R_1$ =0.983 $\\pm$0.030 \\Rsun, $R_2$ =0.901$\\pm$0.026 \\Rsun. Both the primary and secondary stars' radii are 10 \\% and 57\\% larger than those of zero-age-main-sequence stars with the same masses. This discrepancy may be arisen from the large spot coverage of both stars. 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