  We report the observations of the highly active FRb20201124A with the
upgraded Giant Metrewave Radio Telescope at 550-750~MHz. These observations in
the incoherent array mode simultaneously provided an arcsecond localization of
bursts from \rss, the discovery of persistent radio emission associated with
the host galaxy, and the detection of 48 bursts. Using the brightest burst in
the sample ($F= 108~{\rm Jy~ms}$) we find a structure-maximizing dispersion
measure of $410.8 \pm 0.5~{\rm pc~cm}^{-3}$. We find that our observations are
complete down to a fluence level of $10~{\rm Jy~ms}$, above which the
cumulative burst rate scales as a power-law $R(>\!F) = 10~{\rm hr}^{-1}
\left(F/10\mathrm{~Jy~ms}\right)^{\gamma}$ with $\gamma = -1.2 \pm 0.2$. We
find that the bursts are on average wider than those reported for other
repeating FRBs. We find that the waiting time between bursts is well
approximated by an exponential distribution with a mean of $\sim 2.9$ min
during our observations. We searched for periodicities using both a standard
Fourier domain method and the Fast Folding Algorithm, but found no significant
candidates. We measure bulk spectro-temporal drift rates between $-0.75$ and
$-20~{\rm MHz~ms}^{-1}$. Finally, we use the brightest burst to set an upper
limit to the scattering time of 11.1~ms at 550~MHz. The localization of
FRB20201124A adds strength to the proof-of-concept method described in our
earlier work and serves as a potential model for future localizations and
follow-up of repeating FRBs with the uGMRT.
