The galaxy presents a flattened, disk-like structure, viewed at a significant inclination. Its overall color suggests a moderate mix of stellar populations, with a noticeable concentration of bluer light along the disk, potentially indicating regions of ongoing star formation. The disk exhibits some subtle irregularities, hinting at possible internal structures or minor gravitational interactions. There is a lack of a prominent bulge component and a general smoothness to the light distribution, suggesting it is likely a spiral galaxy with a small bulge, or possibly a lenticular galaxy. There are also subtle indications of disturbances and a possible tidal feature in the disk.
