The galaxy presents as an edge-on spiral galaxy, characterized by a distinct flattened disk. A prominent central bulge dominates the galaxy's core, exhibiting a concentrated luminosity gradient. The bulge appears primarily smooth with a rounded structure. A faint, extended halo might be suggested by the diffuse light extending beyond the main disk.

The galaxy is relatively compact. There are possible indications of ongoing star formation in the disk, which might be implied by some bluer hues in the galactic plane. No clear evidence of a major merger event is observed, and the disk appears relatively undisturbed.
