  Drift scan observations provide the broad sky coverage and instrumental
stability needed to measure the Epoch of Reionization (EoR) 21-cm signal. In
such observations, the telescope's pointing center (PC) moves continuously on
the sky. The Tracking Tapered Gridded Estimator (TTGE) combines observations
from different PC to estimate $P(k_{\perp}, k_{\parallel})$ the 21-cm power
spectrum, centered on a tracking center (TC) which remains fixed on the sky.
The tapering further restricts the sky response to a small angular region
around TC, thereby mitigating wide-field foregrounds. Here we consider $154.2
\, {\rm MHz}$ ($z = 8.2$) Murchison Widefield Array (MWA) drift scan
observations. The periodic pattern of flagged channels, present in MWA data, is
known to introduce artefacts which pose a challenge for estimating
$P(k_{\perp}, k_{\parallel})$. We demonstrate that the TTGE is able to recover
$P(k_{\perp}, k_{\parallel})$ without any artefacts, and estimate $P(k)$ within
$5 \%$ accuracy over a large $k$-range. We also present preliminary results for
a single PC, combining 9 nights of observation $(17 \, {\rm min}$ total). We
find that $P(k_{\perp}, k_{\parallel})$ exhibits streaks at a fixed interval of
$k_{\parallel}=0.29 \, {\rm Mpc}^{-1}$, which matches $\Delta \nu_{\rm
per}=1.28 \, {\rm MHz}$ that is the period of the flagged channels. The streaks
are not as pronounced at larger $k_{\parallel}$, and in some cases they do not
appear to extend across the entire $k_{\perp}$ range. The rectangular region
$0.05 \leq k_{\perp} \leq 0.16 \, {\rm Mpc^{-1}}$ and $0.9 \leq k_{\parallel}
\leq 4.6 \, {\rm Mpc^{-1}}$ is found to be relatively free of foreground
contamination and artefacts, and we have used this to place the $2\sigma$ upper
limit $\Delta^2(k) < (1.85 \times 10^4)^2\, {\rm mK^2}$ on the EoR 21-cm mean
squared brightness temperature fluctuations at $k=1 \,{\rm Mpc}^{-1}$.
