Fig. 6.

Panel a: surface brightness profiles along slits, parallel to the x-axis of Fig. 4a. The black line crosses the centre of the galaxy, while the rest of them, from top to bottom, were taken 314, 6
9, and 10″above (red lines) and below (blue lines) it. Panel b: unsharped masked image of the galaxy. Characteristic distances from the galactic centre are indicated in both panels with dashed perpendicular lines, which correspond to morphological features discussed in the text.
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