The galaxy presents as a relatively smooth, disk-like structure, viewed at an oblique angle, but not quite edge-on. The central bulge appears prominent and has a yellowish hue, suggesting an older stellar population. The disk surrounding the bulge shows a subtle color gradient, transitioning from yellowish-green in the inner regions to a slightly bluer tint farther out. This potentially indicates ongoing star formation in the outer disk. There are no obviously distinct spiral arms visible in the image, and it appears largely undisturbed, with no prominent signs of tidal interactions or major mergers. The galaxy appears to be in a relatively quiescent state regarding star formation activity, but is still actively forming stars to some degree.
