  We investigate a possibility that a recently reported radio transient in M81,
VTC J095517.5+690813, is caused by an accretion-induced collapse of a white
dwarf. It became bright in radio but no associated optical transient was
discovered. The accretion-induced collapse is predicted to be radio bright but
optically faint, satisfying the observed property. We compare predicted radio
emission from the accretion-induced collapse with that of VTC J095517.5+690813
and show that it can be reasonably explained by the accretion-induced collapse.
Although it is difficult to firmly conclude that VTC J095517.5+690813 is an
accretion-induced collapse, our study shows that radio-bright transients
without an optical counterpart could still be related to stellar deaths.
