The galaxy presents as a lenticular or edge-on spiral type. Its apparent shape is elongated, suggesting we are viewing a disk-like structure nearly edge-on. The central bulge is prominent and appears to be composed of older stellar populations, exhibiting a yellowish hue. Moving outward from the bulge, the disk displays a bluer coloration, which may indicate the presence of ongoing star formation activity. However, the arms are not distinct, and there is a relatively smooth appearance in the disk, which is typical for a lenticular galaxy. There is no strong evidence of active galactic nuclei activity and no major disturbances or mergers, though subtle irregularities in the disk shape could suggest a history of minor interactions. The overall structure of the galaxy appears to be relatively undisturbed, consistent with an evolved system undergoing more passive star formation.
