  In the current letter, we study isotropic static spherically symmetric
gravastars without charge under the framework of braneworld gravity
(dimensionally reduced RS-II braneworld with positive brane tension) using the
metric potential of Kuchowicz type (which is physically acceptable,
non-singular and stable) in the Mazur-Motolla conjuncture. We derived the
Kuchowicz free parameters from the junction conditions assuming Schwarzschild
vacuum without cosmological constant. As well, we assume that the interior is
filled with Dark Energy (DE-like) fluid, shell with ultrarelativistic stiff
fluid. Adopting this conditions, we probed several physical aspects of the
gravastars, such as proper length, shell energy and entropy, surface redshift
and adiabatic index, interior region mass.
