The galaxy presents as a lenticular or possibly spiral galaxy viewed nearly edge-on. A bulge component is visible, appearing roughly spherical and yellow, indicating an older stellar population. A faint, elongated disk extends beyond the bulge, exhibiting a slightly bluer hue. This suggests the presence of some younger stars or ongoing, but potentially minimal, star formation within the disk. There is no visual evidence of strong spiral arm structure or significant dust lanes. The overall morphology suggests a galaxy with a substantial evolved stellar population and a relatively quiescent star formation history. There are no clear signs of ongoing mergers or major disturbances impacting the galactic structure.
