  Eclipsing binary systems hold a central position within astrophysics in that
the fundamental parameters of stars can be determined by direct observations.
The simultaneous analyses of high-quality space observations, combined with
ground-based photometric data, have allowed more sensitive detection of
fundamental stellar parameters by multicolor photometry. In the paper, the
fundamental parameters of the component stars for the V1175 Cas binary system
were sensitively obtained by a simultaneous analysis of the Transiting
Exoplanet Survey Satellite (TESS) light curve, and new CCD observations in {\it
BVRI} filters obtained with a 60 cm robotic telescope at the TUBITAK National
Observatory. Following the analysis, the masses and radii of the primary and
secondary binary components were determined as $M_{1}= 1.64\pm 0.04\,M_\odot$,
$M_{2}= 1.63\pm0.07\,M_\odot$, and $R_{1}=1.77\pm 0.05\,R_\odot$, $R_{2}=
1.77\pm 0.25\,R_\odot$, respectively. Moreover, the distance of V1175 Cas was
computed as $280\pm32$ pc. The photometric analysis reveals that the components
of the system are in a similar evolutionary state. The primary and secondary
components exhibit nearly the same masses, while their radii are perfectly
matched. Additionally, the ages of the components are also consistent within
the statistical uncertainties. Consequently, the system's overall age is
assessed to be approximately $750\pm70$ Myr.
