Spatially resolved stellar population properties of GAMA 526784 derived using the DAP routine. Top row, left to right: stellar surface mass density (Σ_⋆), mass-weighted age (t_M), and mass-weighted metallicity ([M/H]_M). Bottom row, left to right: light-weighted age (t_L), light-weighted metallicity ([M/H]_L), and colour excess (E(B − V)). Inset panels show the property gradients measured along the two rectangles overlaid on the maps, with grey bands indicating the measurement uncertainties. The maps and profiles reveal a central region that is both more massive and metal-rich compared to the outskirts. Additionally, the western side of the galaxy appears younger and dustier, coinciding with the location of newly formed star clusters.