The observed galaxy presents as an edge-on spiral galaxy, exhibiting a prominent central bulge. The bulge appears relatively smooth and centrally concentrated with a color gradient towards redder hues, indicative of an older stellar population. Extending outwards from the bulge are fainter, bluish-tinged features suggesting a disk component. The disk appears quite thin, characteristic of late-type spiral galaxies observed edge-on. There are possible signs of dust lane obscuration, which might contribute to the mottled appearance in the lower portion of the galactic disk. There is no obvious sign of interaction or merging with another galaxy. The overall morphology points toward a relatively undisturbed, disk-dominated system seen at a significant cosmological distance.
