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Comprehensive analysis of optical spectroscopy and space photometry of thesolar type eclipsing binary system KIC\,4832197 is presented. The system iscomposed of F7V + F9V components with masses of $M_{1}=1.16\pm0.12~M_{\odot}$,$M_{2}=1.07\pm0.10~M_{\odot}$ and radii of $R_{1}=1.26\pm0.04~R_{\odot}$,$R_{2}=1.03\pm0.03~R_{\odot}$. Position of the components on$Log~T_{eff}-Log~L/L_{\odot}$ plane suggests an age of $2.8\pm0.8~Gyr$ for thesystem. Inspection of out-of-eclipse brightness in time reveals wave-likevariability pattern, whose amplitude and shape quickly change in order of days.Frequency analysis of this variability results in two significant peaks inamplitude spectrum, which are interpreted as rotational modulation of spots onthe components. Assuming both spots are on the same component, a lower limitfor differential rotation coefficient is computed as $k=0.12$, which is weakercompared to the solar value of $k_{\odot} = 0.189$.

Solar-type eclipsing binary KIC 4832197: Physical properties and intrinsic variability of the components