The galaxy presents as a flattened, elongated structure, indicative of a disk galaxy viewed nearly edge-on from our vantage point. It displays a central bulge that appears relatively smooth and indistinct. The disk itself shows a mottled texture, potentially indicative of spiral arm structure, although the near edge-on view makes discerning distinct arms challenging.

There appears to be some evidence of dust lanes running parallel to the galactic plane, particularly in the central regions, obscuring some of the starlight. The galaxy exhibits a colour gradient. The central bulge appears yellower, suggestive of an older stellar population. The outer regions of the disk show hints of bluer hues, indicating the presence of younger, hotter stars.

The overall morphology suggests an active, star-forming galaxy, possibly in the transition phase.
