  Recently discovered regular X-ray bursts known as quasi-periodic eruptions
have a proposed model that suggests a tidal stripping white dwarf inspiralling
into the galaxy's central black hole on an eccentric orbit. According to this
model, the interaction of the stripping white dwarf with the central black hole
would emit gravitational wave signals as well, their detection can help explore
the formation mechanism of quasi-periodic eruptions and facilitate
multi-messenger observations. In this paper, we aim to perform a preliminary
study of the gravitation wave observation of TianQin on this stripping white
dwarf model. We investigated the horizon distance of TianQin on this type of
gravitation wave signal and found it can be set to 200Mpc. We also find that
those stripping white dwarf model sources with central black hole mass within
$10^4\sim10^{5.5}M_\odot$ are more likely to be detected by TianQin. We
assessed the parameter estimation precision of TianQin on those stripping white
dwarf model sources. Our result shows that, even in the worst case, TianQin can
determine the central black hole mass, the white dwarf mass, the central black
hole spin, and the orbital initial eccentricity with a precision of $10^{-2}$.
In the optimistic case, TianQin can determine the central black hole mass and
the white dwarf mass with a precision of $10^{-7}$, determine the central black
hole spin with a precision of $10^{-5}$, and determine the orbital initial
eccentricity with a precision of $10^{-8}$. Moreover, TianQin can determine the
luminosity distance with a precision of $10^{-1}$ and determine the sky
localization with a precision of $10^{-2}\sim10$ $\rm deg^2$.
