CGCG 012-070 galaxy. Top left panel: 2.0μm continuum image of CGCG 012-070, obtained from the NIRSpec data cube. Other top panels: Flux distributions of the [Fe II]1.6440μm, Paα, and H₂2.1218 μm emission lines. Gray regions represent masked out areas where the S/N < 3 and regions outside the NIRSpec FoV. The cross marks the position of the continuum peak. Bottom panel: Observed spectrum (in black), integrated over a 0$\stackrel{″}{.}$25 radius nuclear aperture (black circle in the top left panel). The red curve represents the stellar population (SP) model, while the blue curve shows the gas contribution (observed - SP). Vertical lines mark the position of the main emission lines.