  We present a study of eclipsing binary J064726.39+223431.6 using spectra from
the LAMOST-MRS and TESS photometry. We use full-spectrum fitting to derive
radial velocities and spectral parameters: ${T_{\rm eff}}_{A,B}=6177,\,5820$ K,
$v \sin{i}_{A,B}=59,\,50~\kms$ and ${\rm [Fe/H]}_{A,B}=-0.19$ dex. The orbital
solution and light curve analysis suggest that it is a close pair of fast
rotating stars on circular orbit. We measure their masses to be
$M_{A,B}=1.307\pm0.007,\, 1.129\pm0.005\,M_\odot$ and their radii to be
$R_{A,B}=1.405\pm0.052,\, 1.219\pm0.060\,R_\odot$ resulting in surface
gravities of $\log{g}_{A,B}=4.259\pm0.033,\,4.319\pm0.042$ (cgs). Theoretical
models cannot match all of these properties, predicting significantly higher
${T_{\rm eff}}$ for a given metallicity. Derived age of the system 1.56 Gyr
indicates that both components are younger than Sun, which contradicts to much
longer orbit's circularisation timescale.
