  We present results of an asteroseismic study on the $\gamma$ Dor type {\it
Kepler} target KIC\,6462033. {\it Kepler} photometry is used to derive the
frequency content and principal modes. High-dispersion ground-based
spectroscopy is also carried out in order to determine the atmospheric
parameters and projected rotational velocity. From an analysis of the {\it
Kepler} long cadence time series, we find that the light curve of KIC\,6462033
is dominated by three modes with frequencies $f_{1}$=0.92527, $f_{2}$=2.03656
and $f_{3}$=1.42972 d$^{-1}$ as well as we detect more than a few hundreds of
combination terms. However, two other independent frequencies appear to have
lower amplitudes in addition to these three dominant terms. No significant
peaks are detected in the region $>$ 5 d$^{-1}$. We therefore confirm that
KIC\,6462033 pulsates in the frequency range of $\gamma$ Dor type variables,
and a future study will allow us to investigate modal behaviour in this star.
