The galaxy presents as a thin, elongated disk structure seen edge-on. The central bulge appears subtly brighter and more condensed than the outer regions of the disk. There is evidence of some dust lane absorption along the galactic plane. The overall color of the galaxy suggests a population of older stars, primarily. There is limited, if any, indications of spiral arm structure visible due to the edge-on orientation, and I am also unable to discern whether or not there is any bar structure present, or any indications of ongoing mergers or tidal disturbances.
