  Galaxy clusters are located at the nodes of cosmic filaments and therefore
host a lot of hydrodynamical activity. However, cool core clusters are
considered to be relatively relaxed systems without much merging activity. The
Abell 85 cluster is a unique example where the cluster hosts both a cool core
and multiple ongoing merging processes. In this work, we used 700 MHz uGMRT as
well as MeerKAT L-band observations, carried out as part of the MGCLS, of the
Abell 85. We reconfirm the presence of a minihalo in the cluster centre at
700MHz that was recently discovered in MGCLS. Furthermore, we discovered a
radio bridge connecting the central minihalo and the peripheral radio phoenix.
The mean surface brightness, size and flux density of the bridge at 700 MHz is
found to be $\sim 0.14\ \mu$Jy/arcsec$^2$, $\sim 220$ kpc and $\sim 4.88$ mJy,
respectively, with a spectral index of $\alpha_{700}^{1.28} = -0.92$. Although
the origin of the seed relativistic electrons is still unknown, turbulent
re-acceleration caused by both the spiralling sloshing gas in the intracluster
medium (ICM) and the post-shock turbulence from the outgoing merging shock
associated with the phoenix formation may be responsible for the bridge.
