The galaxy appears to be a spiral galaxy, viewed nearly edge-on. A central bulge is visible, exhibiting a yellow-orange hue, suggestive of an older stellar population. Extending outwards from the bulge are fainter regions, which likely represent the galactic disk. Subtle color variations within the disk indicate areas of ongoing star formation, possibly traced by bluer regions. The galaxy is not entirely smooth; some irregularities and possible distortions are apparent within the disk. The overall structure seems relatively undisturbed, exhibiting only minor disturbances. The galaxy shows no signs of a major merger event.
