  Eclipsing binary systems have a unique feature, which enables scientists to
obtain precise fundamental star parameters, which opens to greater area of
astrophysics studies. In this study, we have derived the fundamental
parameters, the evolutionary status, and the birthplace of V454 Aur in the
Galaxy by combining radial velocity, photometric, and spectral energy
distribution data. We have updated ephemerides and period of V454 Aur as
$2458850.80136_{-0.00001}^{\,+0.00001}$ and
$27.0198177_{-0.0000003}^{\,+0.0000003}$, respectively. We obtain
$1.173^{\,+0.016}_{-0.016}$ $M_\odot$ and $1.203^{\,+0.022}_{-0.026}$ $R_\odot$
for the primary component and $1.045^{\,+0.015}_{-0.014}$ $M_\odot$ and
$0.993^{\,+0.034}_{-0.027}$ $R_\odot$ for the secondary component. The
effective temperatures for the components are accurately determined via SED
data as $6250^{\,+150}_{-150}$ K and $5966^{\,+109}_{-89}$ K for the primary
component and the secondary component, respectively. The metallicity of the
components is derived from evolutionary tracks, which implies slightly higher
than Solar metallicity. According to analysis, the components of V454 Aur are
on the main sequence. Our distance calculation for the system is, which is
$65.07^{\,+2}_{-3}$ pc, in excellent agreement with \textit{Gaia} astrometric
data, which is $65.07^{\,+0.09}_{-0.09}$ pc. The current age of the system is
$1.19_{-0.09}^{\,+0.08}$ Gyr, and it will start to mass transfer between
components in 5 Gyr from now on. Dynamical orbital analysis shows that V454 Aur
follows a boxy pattern around the Galactic centre and is a member of the
thin-disc component of the Galaxy. Considering the age and metallicity of this
system, it was found to have formed just outside the Solar circle.
