  We show that observed properties of the low luminosity GRB171205A and its
afterglow, like those of most other low-luminosity (LL) gamma ray bursts (GRBs)
associate with a supernova (SN), indicate that it is an ordinary SN-GRB, which
was produced by inverse Compton scattering of glory light by a highly
relativistic narrowly collimated jet ejected in a supernova explosion and
viewed from a far off-axis angle. As such, VLA/VLBI follow-up radio
observations of a superluminal displacement of its bright radio afterglow from
its parent supernova, will be able to test clearly whether it is an ordinary
SN-GRB viewed from far off-axis or it belongs to a distinct class of GRBs,
which are different from ordinary GRBs, and cannot be explained by standard
fireball models of GRBs as ordinary GRBs
