Top left: The continuum-subtracted images of the galaxy. Top right: The identified PAH clouds using SCIMES. The flagged clouds are in grey, non-flagged in green, and PAH clouds with CO cloud counterparts in red. Middle left: Sigma_mol violin plots per galactic environment for the specific galaxy (transparent), and the full sample (colored). The median values and number of PAH clouds per environment are also represented in the plot. Middle center: log(M_mol )-log(R_eq) scaling relation for the PAH clouds in the galaxy (blue), clouds per galactic environment in the galaxy (see colors in plot), and for the full sample (black). The median values are also represented in the plot per galactic environment. Middle right: The global mass spectra (black), galaxy-specific mass spectra (blue), and per galactic environment in the galaxy. The fit values for the galaxy-specific mass spectra are displayed in the plot. Bottom: The \sigmol\ (left), \Mmol\ (center), and \Reff\ (right) as a function of R_gal. A scatterplot of the PAH clouds, colored by the density of clouds, is also represented in the plots. The running galaxy median (filled blue circles) is plotted for a bin width of 0.1 R_e. The grey-shaded region represents the interquartile range of the medians per galaxy. The error bars on the median are the standard errors (1.253 x sigma/sqrt(N)), where N is the number of clouds contributing to a specific bin. The blue and black dashed lines represent the median property of the galaxy and the full sample, respectively.