The galaxy appears to be a spiral galaxy, seen nearly edge-on from our perspective. It exhibits a prominent central bulge which is elliptical in shape. The bulge displays a yellowish hue, suggesting an older stellar population is more dominant. Extending outward from the bulge are the galactic disk, which have a bluer tint due to the presence of younger stars. The disk material appears relatively smooth, and with a hint of obscuration near the midplane, implying the presence of dust lanes. The galaxy appears undisturbed with no tidal tails or signs of major mergers or interactions.
