The galaxy presents as a lenticular or possibly an elliptical galaxy with a relatively smooth light distribution. It appears elongated in shape, with an axial ratio indicating it is significantly inclined to our line of sight. The central bulge is prominent and yellowish in color, suggesting an older stellar population. The galaxy exhibits a faint disk component surrounding the bulge with a slightly bluer hue, hinting at a small amount of ongoing star formation activity. There are no clear signs of strong spiral arm structure or significant dust lanes visible. The overall morphology suggests that the galaxy is likely evolved and relatively quiescent. No tidal features or other signs of recent major merger activity are discernible.
