The observed galaxy presents as an edge-on spiral, exhibiting a clear disk-like structure. The central bulge appears prominent and elongated, possibly with a somewhat boxy morphology. Dust lanes are visible along the galactic plane, obscuring some of the light from the bulge. There's evidence of ongoing star formation within the disk, indicated by a slightly bluer hue extending outwards from the central regions, with reddish areas also visible. The disk appears relatively undisturbed, without any signs of a major merger event. The galaxy seems to be a relatively massive and actively star-forming system.
