Joint posterior distributions of the main physical properties in our analysis, the best-fit SED, and the recovered SFH for a selected pixel bin of TNG414917 with the O4 orientation index. The corner plot displays the posterior distributions of ${\widehat{\tau }}_{\mathrm{dust},2}$, sSFR, t_★,  mw, Z_★, and Σ_★. Contours enclose the 20%, 50%, and 80% of the total data, while the vertical dashed black lines mark the median values for each parameter. The median and the 16^th–84^th percentile range for each physical property are given at the top of the corresponding posterior distribution. The Spearman’s correlation coefficient, ρ, quantifies the strength of correlation between two posterior distributions. Top right: Comparison of the input photometric data (red points) to the best-fit SED model (blue line). Bottom right: Subpanel illustrating the absolute residuals defined as ΔF_ν = log₁₀(fit/ground truth). The photometric uncertainties are not visible in the plot because they are smaller than the symbol size. Bottom: Posterior distribution of the SFH.