The galaxy presents as a lenticular or spiral galaxy viewed edge-on from our line of sight. The central bulge is a bright, concentrated region, indicating a substantial population of older stars. The disk appears elongated and relatively smooth, suggesting a lack of prominent spiral arm structure. The overall color profile indicates a galaxy with a mix of stellar populations, possibly with ongoing, but limited, star formation. There is no clear evidence of a strong central bar feature. The disk shows subtle variations in color and brightness, perhaps suggesting dust lanes or subtle spiral structure. The outer regions of the disk fade gradually into the background, indicating a smooth density profile. There appear to be no signs of major mergers or significant tidal disturbances. It is likely a fairly massive galaxy with a substantial stellar mass.
