  In this article, we anchor our analysis on the premise that the presence of a
photon sphere is an intrinsic characteristic of any ultra-compact gravitational
structure with spherical symmetry. Utilizing the concept of a topological
photon sphere, we categorize the behaviors of diverse gravitational models
based on the structure of their photon spheres. This innovative approach
enables us to define boundaries for black hole parameters, which subsequently
allows us to classify the model as either a black hole or a naked singularity.
Indeed, we will demonstrate that the existence of this reciprocal relationship
between the gravitational structure and the presence of a photon sphere offers
a unique advantage that can be directly and inversely harnessed. Furthermore,
we present a precise correlation between the behavior of the defined effective
potential and the total topological charge for each model. Through an
independent examination of the effective potential, we show that a
gravitational model typically exhibits naked singularity behavior when at least
one effective potential minimum (a stable photon sphere) protrudes beyond the
event horizon. Finally, we will compare the effect of adding perfect fluid dark
matter to the models under study and observe the impact of this quantity on the
behavior of the photon sphere and the extent of their dominance.
