  Gamma-ray bursts are traditionally classified as short and long bursts based
on their $T_{\rm 90}$ value (the time interval during which an instrument
observes $5\%$ to $95\%$ of gamma-ray/hard X-ray fluence). However, $T_{\rm
90}$ is dependent on the detector sensitivity and the energy range in which the
instrument operates. As a result, different instruments provide different
values of $T_{\rm 90}$ for a burst. GRB 210217A is detected with different
duration by {\it Swift} and {\it Fermi}. It is classified as a long/soft GRB by
{\it Swift}-BAT with a $T_{\rm 90}$ value of 3.76 sec. On the other hand, the
sub-threshold detection by {\it Fermi}-GBM classified GRB 210217A as a
short/hard burst with a duration of 1.024 sec. We present the multi-wavelength
analysis of GRB 210217A (lying in the overlapping regime of long and short
GRBs) to identify its actual class using multi-wavelength data. We utilized the
$T_{\rm 90}$-hardness ratio, $T_{\rm 90}$-\Ep, and $T_{\rm 90}$-$t_{\rm mvts}$
distributions of the GRBs to find the probability of GRB 210217A being a short
GRB. Further, we estimated the photometric redshift of the burst by fitting the
joint XRT/UVOT SED and place the burst in the Amati plane. We found that GRB
210217A is an ambiguous burst showing properties of both short and long class
of GRBs.
