The galaxy presents as a lenticular or early-type spiral, observed at a considerable inclination. It exhibits a prominent central bulge that appears relatively smooth and featureless in the available image. Surrounding the bulge, a faint disk is suspected, but detailed spiral arm structure is not readily discernible. There is evidence of some form of disturbance that is slightly affecting the morphology of the galaxy, the disk appears disturbed. The galaxy shows a predominantly older stellar population within the bulge, which is implied by its smoother appearance and lack of significant blue color. There is also evidence of ongoing star formation. There is very little active galactic nuclei activity. Overall, the galaxy suggests a system that is transitioning, where star formation is winding down. The absence of strong tidal features or close companion galaxies nearby may rule out major interactions as the primary cause of any disturbance, hinting at internal processes or minor mergers influencing its evolution.
