The galaxy appears to be a spiral, viewed edge-on. A prominent central bulge dominates the galaxy's core, exhibiting a yellowish hue, which might indicate an older stellar population. From the central bulge, a disk extends outwards, appearing relatively smooth. The disk component is noticeably flatter than the bulge, consistent with typical disk galaxy morphology. There is a subtle color gradient within the disk, with the regions closer to the bulge having a more yellowish tint, subtly transitioning towards a bluer hue at the edges of the disk. The dust lane appears to be visible in the disk, and the lack of clumpy features within the disk might suggest that the galaxy is relatively undisturbed. Overall, the galaxy presents a fairly symmetrical and well-defined structure.
