The observed galaxy presents as an edge-on spiral, exhibiting a pronounced dust lane bisecting the central bulge. The bulge itself appears relatively smooth and elongated, suggesting a primarily spheroidal stellar population. The spiral arms are not clearly defined, and the galaxy is not particularly bright, indicating a lower overall star formation rate. There's evidence of a possible tidal tail or disturbed morphology on one side of the galaxy, hinting at a previous or ongoing interaction. The primary color of the galaxy is yellowish, with a hint of bluer colors in the disk, suggesting some younger stellar populations. 
