The galaxy presents as a lenticular or early-type spiral galaxy. It displays a generally smooth, centrally concentrated morphology with a subtle disk-like structure. The core region exhibits a bright, somewhat unresolved bulge. Faint and diffuse spiral arm segments are potentially visible, hinting at a weak disk component. The galaxy's color is bluer towards its central regions, and as we move away from the center, the color slightly reddens. This may indicate older stellar populations. There are no apparent signs of significant tidal disturbances, strong star formation regions, or an active galactic nucleus. Overall, the galaxy appears to be a relatively quiescent system in a late stage of its evolution.
