Best-fit SED model of LACES104037 derived using Prospector, fitted to the existing broadband photometry and IFU spectroscopy. Our spectral fitting results are shown in Table 2. The best-fit SED model yields a reduced chi-square of χ² = 2.93. LACES104037 is characterized by a very young stellar population, with its SED dominated by a moderately evolved component of age ∼16 Myr, while an additional recent starburst within the past ∼1 Myr is required to reproduce the observed spectroscopic and photometric properties.