This appears to be a spiral galaxy with a disk-like structure viewed at an oblique angle, exhibiting a significant tilt relative to our line of sight. The galaxy's morphology is clearly disrupted, indicating possible ongoing or recent interactions with another galaxy. Faint spiral arms are visible, exhibiting a loosely wound structure. One arm is clearly visible, while the other is very difficult to see. The central bulge seems to be present but not the dominant feature of the galaxy. It is of moderate size. There appears to be a bar in the galaxy, but it is hard to tell how strong or weak it is based on the image. Color gradients suggest active star formation regions within the disk, contrasted by older stellar populations in the bulge.
