  In physical science, the concept of \emph{emergence} is often used to
describe phenomena that occur at macroscopic scales but not at microscopic
scales. The latter is usually referred to as a \emph{fundamental property} and
the former as an \emph{emergent property}. In this paper, noncommutative
geometry, often viewed as an offshoot of string theory, is the primary
fundamental theory that gives rise to macroscopic wormholes and their
properties, thereby becoming an emergent phenomenon. As a consequence of these
considerations, we will reexamine the boundary conditions that characterize a
Morris-Thorne wormhole, resulting in a modification of the wormhole structure.
