  Naked singularities form during the gravitational collapse of inhomogeneous
matter clouds. The final nature of the singularity depends on the initial
conditions of the matter properties and types of matter profiles. These naked
singularities can also be divided into two types: null-like and timelike
singularities. The spacelike singularity of the Schwarzschild black hole can be
distinguished from the null and timelike naked singularity spacetimes. In light
of this, we investigate the precession of timelike bound orbits in the null
naked singularity spacetime, as well as tidal force effects and geodesic
deviation features. As a result, we find that the orbital precession of the
timelike bound orbits in null naked singularity spacetime could be
distinguished from the Schwarzschild precession case. The radial component of
the tidal force has an intriguing profile, whereas the angular component has a
profile which is comparable to that of a Schwarzschild black hole scenario. The
geodesic deviation equation is then solved numerically, yielding results that
resemble a Schwarzschild black hole. These characteristic features can then be
used to discern amongst these singularities.
