The galaxy presents as an elongated, disk-like structure, viewed at a moderate inclination relative to our line of sight. It appears to be relatively smooth in texture, suggesting it is most likely an early-type spiral or lenticular galaxy. There is a bulge that shows a concentration of light toward the center, indicating a possible supermassive black hole. The galaxy exhibits color variations, with a yellowish-white central region and slightly bluer outer regions. This potentially indicates younger star formation in the disk compared to the center. Some minor disturbances are present, though the object does not present as a recent major merger.
