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.
Categories: astro-ph.HE