This galaxy presents as a disk galaxy, possibly seen at an oblique angle, not quite edge-on, and not quite face-on. The central bulge appears prominent and exhibits a yellowish-white hue, suggesting an older stellar population. The disk is characterized by a more bluish tint, which is indicative of ongoing star formation and the presence of younger, hotter stars. The disk appears relatively smooth, with only subtle hints of spiral arm structure. There are regions in the disk which suggest the presence of dust lanes, obscuring some of the background light. Based on its morphology, the galaxy does not appear to be undergoing any major mergers, although there might be minor tidal features or disturbances that are hard to discern at the current image resolution.
