  We present the broadband X-ray study of the BeXRB pulsar IGR J06074+2205
using NuSTAR observations. The temporal and spectral characteristics of the
source are investigated. We detect coherent X-ray pulsations of the source and
determine the spin period evolution. Using the current spin period data of the
source, we show that the source is spinning down at 0.0202(2)\; s\; $day^{-1}$.
The pulse profiles are found to evolve with energy and luminosity. Another
interesting feature of the source is that the pulse profiles are dual peaked.
The dual-peaked pulse profile is characterized by a decreasing secondary peak
amplitude with increasing energy. We also observed a proportionate increase in
the primary peak amplitude as the energy increases. The pulse fraction exhibits
an overall increasing trend with the energy. The X-ray continuum of the source
indicates the existence of a characteristic absorption feature with a centroid
energy $\sim 55$ keV, which may be interpreted as a cyclotron line. We estimate
the corresponding magnetic field strength to be $\sim4.74\times10^{12}$ G. A
peculiar `10 keV' absorption feature is observed in the X-ray spectra of the
second observation.The luminosity measurements predict that the source may be
accreting in the sub-critical regime.
