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The ${\\it Kepler}$ light curve of this system was simultaneously solved with the radial-velocity data given by Matson et al. (2017). The results indicate that the binary star is a short-period semi-detached system with fundamental parameters of $M_1$ = 1.66$\\pm$0.04 M$_\\odot$, $M_2$ = 0.215$\\pm$0.006 M$_\\odot$, $R_1$ = 1.53$\\pm$0.02 R$_\\odot$, $R_2$ = 1.33$\\pm$0.02 R$_\\odot$, $L_1$ = 5.0$\\pm$0.6 L$_\\odot$, and $L_2$ = 0.96$\\pm$ 0.09 L$_\\odot$. 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