The galaxy presents as a flattened, disk-shaped system, viewed nearly edge-on from our perspective. The central region exhibits a yellowish hue, suggestive of an older stellar population and potentially a bulge component. Moving outwards from the center along the galactic plane, the color transitions to a bluer shade, indicating younger, hotter stars and active star formation regions within the disk.

The disk appears somewhat disturbed or warped, possibly due to past interactions or ongoing accretion events. Faint traces of what might be spiral arm structures are hinted at in the bluer regions, although the edge-on viewing angle obscures a clear view. There is a subtle dust lane obscuring some of the starlight.
