The galaxy appears to be a spiral galaxy, viewed at an oblique angle, nearing edge-on. There is a prominent central bulge that appears bright. It's difficult to discern distinct spiral arms due to the viewing angle, but there's a clear disk component that extends outwards from the bulge on either side.

The galaxy exhibits a bluish tint in the outer regions of the disk. This suggests the presence of younger, hotter stars. Dust lanes appear to be present along the disk. There is some indication of a possible bar-like structure present in the central region, though it isn't particularly strong. The galaxy also appears to have a faint tidal feature or asymmetry in its structure, possibly indicating a past or ongoing minor interaction with another galaxy.
