The galaxy appears as a flattened, disk-shaped structure viewed nearly edge-on. Its central bulge is indistinct, with a diffuse, smooth light distribution exhibiting a subtle concentration towards the center. The disk component displays a faint, bluish hue, suggesting the presence of relatively young, hot stars and active star formation, though the rate appears low. There is no obvious spiral arm structure visible, indicating a potentially disturbed morphology. The overall shape is elongated, with the major axis significantly exceeding the minor axis. Some faint disturbances are visible along the main axis, which could be evidence of minor interactions.
