  Comprehensive analysis of optical spectroscopy and space photometry of the
solar type eclipsing binary system KIC\,4832197 is presented. The system is
composed 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 the
system. Inspection of out-of-eclipse brightness in time reveals wave-like
variability pattern, whose amplitude and shape quickly change in order of days.
Frequency analysis of this variability results in two significant peaks in
amplitude spectrum, which are interpreted as rotational modulation of spots on
the components. Assuming both spots are on the same component, a lower limit
for differential rotation coefficient is computed as $k=0.12$, which is weaker
compared to the solar value of $k_{\odot} = 0.189$.
