The observed galaxy exhibits a clear disk morphology, viewed at an intermediate angle, not quite edge-on. The central region is noticeably brighter and more concentrated, with a distinct yellowish hue suggestive of an older stellar population. Extending outward from this central bulge are fainter, bluer regions, possibly indicative of more recent star formation occurring within the disk. There is evidence of some disturbance to the overall structure, possibly hinting at minor tidal interactions or an ongoing minor merger event. The disk appears somewhat patchy, and there may be some faint, elongated features extending beyond the main body of the galaxy, but not enough to be sure if the galaxy is interacting with another or there is a disturbance within the disk.
