  We present the spectral and timing study of the bright NS-LMXB GX 5-1 using
\textit{\textit{AstroSat}/LAXPC} and \textit{SXT} observations conducted in the
year 2018. During the observation, the source traces out the complete HB and NB
of the Z-track in the HID. Understanding the spectral and temporal evolution of
the source along the 'Z' track can probe the accretion process in the vicinity
of a neutron star. Spectral analysis was performed in the 0.7-20 keV energy
range for different segments in the HID using a multi-temperature disc black
body with an average temperature, $kT_{in} \sim$0.46 and a thermal
Comptonization model. It is found that the optical depth of the corona drops
from $\sim$6.68 in HB to $\sim$2.74 in NB. The Timing analysis using the LAXPC
instrument indicates the presence of quasi-periodic oscillations in HB, NB, and
the hard apex of the Z-track. The observed QPO frequencies are similar to the
characteristic frequencies of horizontal branch and normal branch oscillations.
The HBO frequency increase from $\sim$12-46 Hz towards the hard apex. The
timing studies conducted in soft and hard band indicate the association of HBO
and NBO origin with the non-thermal component. Further research could explore
the implications of this relationship for understanding the dynamics of
accretion onto neutron stars.
