The galaxy presents as a disk galaxy, viewed nearly edge-on from our line of sight. The central bulge appears somewhat prominent, suggesting a moderate-sized central concentration of stars. There's a relatively high degree of dust attenuation along the plane of the disk, indicating a significant amount of interstellar material obscuring light from stars within the disk. Some minor disturbances are observed along the galaxy's edges, particularly on one side, indicating a potential ongoing interaction or past merger event. The overall color suggests a galaxy with a mix of stellar populations; the bulge shows a yellower hue possibly due to an older population, while the disk exhibits bluer tinges, hinting at more recent star formation.
