The galaxy presented in this image exhibits a clear disk morphology, viewed nearly edge-on. The disk appears elongated and relatively thin, suggesting a high degree of flattening. Light from the disk appears relatively smooth, with no obvious signs of spiral arm structure.

The central bulge is prominent and appears rounded. The bulge luminosity is significantly brighter than that of the disk, possibly indicating an older stellar population. There are no apparent signs of significant dust lanes obscuring the bulge or the disk. There are no obvious signs of tidal tails or other morphological disturbances, suggesting a quiescent state without recent major mergers or interactions. 
