The galaxy presents as a disk galaxy oriented nearly edge-on from our perspective. The dust lane appears prominent and relatively continuous, bisecting the galaxy's light. There is a central bulge exhibiting a somewhat round morphology. The overall color gradient appears to shift from a bluer hue at the outer edges of the disk to a more reddish-orange color towards the galactic center, indicating potential variations in stellar population age and composition. A small degree of warping might be present in the disk structure, particularly on one end. No strong signs of interactions or major disturbances are immediately apparent. The morphology suggests a system with ongoing or recent star formation.
