The galaxy presents as an edge-on spiral galaxy, exhibiting a flattened disk structure with a central bulge. The disk appears relatively smooth with limited resolved features. The bulge region is concentrated and exhibits a brighter, bluer color profile compared to the disk, suggesting a population of younger stars. There's a slight tilt in the disk's orientation, as the galaxy is not perfectly edge-on. There is no evidence of major morphological disturbances or merging activity. Dust lanes are not clearly resolved within the disk.
