The galaxy appears as an elliptical or lenticular system, showing a relatively smooth light distribution. The central bulge presents a yellowish hue, indicating an older stellar population dominated by evolved stars. Moving outward from the center, the galaxy exhibits fainter, bluer regions, which may signify the presence of younger stars and some ongoing star formation within the galaxy. The galaxy appears elongated, suggesting a flattened or disk-like structure viewed at an angle. There is no obvious sign of spiral arms or a prominent bar, suggesting the disk is relatively smooth or tightly wound. There is no obvious sign of strong gravitational disturbance or interaction with other galaxies.
