The galaxy appears to be a disk galaxy, viewed nearly edge-on. There's a prominent, bright central bulge exhibiting a yellowish hue, suggesting an older stellar population. A dust lane bisects the galaxy horizontally, appearing dark and obscuring light from the bulge. The disk component displays faint extensions on either side of the bulge, showing a bluer color than the bulge, indicating the presence of younger stars. Evidence of minor disturbances can be seen in the warped appearance of the disk, which suggests a possible past interaction or merger event. There is an extension of the top of the warp that appears brighter than other areas of the disk, and a possible companion galaxy near the lower portion of the disk. The overall structure suggests a dynamically active system.
