The galaxy presents as an edge-on spiral galaxy with a prominent disk. The central bulge appears relatively large and elliptical, exhibiting a yellowish-orange hue suggestive of an older stellar population. Dust lanes appear to be present within the disk, causing some obscuration of light from behind. These dust lanes are mottled.

The galaxy's disk shows a slight warp and appears thin. It is relatively smooth in appearance without apparent distinct spiral arms. Some blueish clumps can be seen in the disk, indicating regions of recent star formation. There is no evidence of any major merging events, though some minor disturbance cannot be ruled out. The overall morphology suggests a stable, relatively undisturbed system.
