The galaxy presents an elongated morphology, appearing as an edge-on or highly inclined disk system. A prominent central bulge is evident, displaying a yellowish-orange hue, suggestive of an older stellar population. The galactic disk exhibits a bluer coloration, indicative of ongoing star formation activity. There is a noticeable asymmetry in the disk's structure, potentially resulting from gravitational interactions or internal disturbances. Faint, diffuse features extend outward from the main galactic body, possibly tidal streams or disrupted spiral arms. High likelihood of merging is present, as the galaxy is noticeably disturbed.
