The galaxy presents as an edge-on spiral, exhibiting a clear disk-like structure. A prominent dust lane bisects the galaxy's length, obscuring the central bulge region, which appears relatively small and elongated. There is a subtle color gradient, transitioning from bluer hues at the outer edges of the disk, potentially indicating regions of ongoing star formation, to yellower/whiter tones towards the central region. This could be due to older stellar populations dominating the inner regions. The galaxy's morphology appears relatively undisturbed, with no obvious signs of a major recent merger or tidal interactions. Some irregularities can be seen, possibly due to minor disturbance events. The structure looks to be fairly smooth and integrated.
