  In this study, we investigate the signatures of a non-commutative black hole
solution. Initially, we calculate the thermodynamic properties of the system,
including entropy, heat capacity, and Hawking radiation. For the latter
quantity, we employ two distinct methods: surface gravity and the topological
approach. Additionally, we examine the emission rate and remnant mass within
this context. Remarkably, the lifetime of the black hole, after reaching its
final state due to the evaporation process, is expressed analytically up to a
grey-body factor. We estimate the lifetime for specific initial and final mass
configurations. Also, we analyze the tensorial quasinormal modes using the
6th-order WKB method. Finally, we study the deflection angle, i.e.,
gravitational lensing, in both the weak and strong deflection limits.
