Multi-colour image with red: F277W, green: F150W, and blue: V-band, showing the coverage where all data overlap (the V-band and F277W images were adjusted to show the same spatial coverage, including dither gaps), and individual images shown in insets on the right. The NIRCam data was convolved to a 0.2″ Gaussian PSF. We indicate galactocentric radii r at 3 and 7 kpc. Conspicuous dark features show dusty filaments seen in extinction perpendicular to the disk. We can also notice the presence of star clusters, some obscured by dust, and some are not.