The galaxy presents as an edge-on spiral, with a disk extending horizontally across the field of view. Dust lanes appear prominent, bisecting the galaxy's light and indicating significant obscuration within the plane of the disk. The central bulge appears relatively small and indistinct. Some areas within the galaxy are brighter and bluer, hinting at possible regions of active star formation, although these regions are not very distinct, and their shape is not consistent. The galaxy exhibits a relatively smooth structure and does not show any signs of significant tidal disturbances or interactions. The overall morphology indicates a spiral galaxy with limited bulge prominence, seen edge-on, with some indications of on-going but limited star formation.
