The galaxy presents as a spiral galaxy viewed nearly edge-on. A prominent bulge is observed, exhibiting a smooth, concentrated light profile. The disk is characterized by an extended structure, with dust lanes visible along the plane of the disk. The galaxy appears slightly asymmetrical, possibly due to tidal interactions or internal asymmetries. Indications of star formation regions are present in the disk, appearing as slightly brighter and bluer patches. The disk exhibits a distinct truncation, suggesting a sharp boundary in its star formation activity.
