The two subsamples are split by position on the ﹩{{\rm{log}}}_{10}({M}_{\star ,R\gt 20\,{\rm{kpc}}}/{M}_{\odot })﹩ vs. σ_⋆,cen plane (top left). For galaxies with similar outskirt stellar mass, orange pentagons represent the galaxies with larger inner velocity dispersion (high σ_*), and blue stars represent galaxies with smaller inner velocity dispersion (low σ_*). The background gray circles stand for the total sample. The top-right plot displays the radial profiles of stellar mass density (M_⊙ kpc^–2), with the thick lines representing the median profiles. Using the same color-coding convention, the histograms show the distributions of their physical parameters, including M_* (bottom left), σ_⋆,cen (bottom middle), and redshift (bottom right). Orange solid lines and blue dashed lines correspond to high-σ_* and low-σ_* samples, respectively, and the gray-filled bar is the total sample. The Jupyter notebook for reproducing this figure can be found here: ✎. This repository is also available on Zenodo (https://doi.org/10.5281/zenodo.17979404).