Skaro populates a Milky‑Way–like galaxy with synthetic planetary systems by combining high‑resolution hydrodynamical galaxy formation outputs from the HESTIA simulations with planet population synthesis from the New Generation Planet Population Synthesis (NGPPS) framework. The code assigns planets to stars based on host‑star mass and metallicity, identifies distinct Galactic morphological components (e.g., bulge, thin disk, thick disk, halo), and computes distributions and occurrence rates of planets across these components. It provides routines for data handling, analysis of stellar and planetary populations, and visualization (e.g., radial profiles and spatial maps) to study how exoplanet demographics vary with Galactic environment.