  It is widely believed that the curvature singularities are an artifact of
general relativity and may not exist in the Universe, and likely to be defined
by the quantum gravity. In the absence of successful quantum gravity,
significant attention has been shifted towards the regular models. We present a
five-dimensional ($5D$) rotating regular Myers-Perry like black hole metric
with two rotation parameters ($a,b$) and a free parameter ($k$). Our $5D$
rotating regular metric encompasses $5D$ Myers-Perry black hole which can be
recovered as a special case when $k=0$. The size of the shadow cast by the
black holes is significantly smaller and more distorted when the parameter $k$
is increased.
