The galaxy appears to be a spiral galaxy, viewed at a significant angle, but not fully edge-on.  The disk component dominates the visual appearance. Spiral arms are clearly visible, exhibiting a flocculent morphology with varying degrees of winding. Some of the spiral arms are quite loose and extended.

The central bulge is discernible, moderate in size relative to the disk, though partially obscured.  There is an indication of a faint bar structure across the central region.

There are signs of possible tidal disruption or interaction with another galaxy. There is an extended plume extending from one side of the galaxy, and a portion of the disk appears warped or disturbed. These features may indicate an ongoing or recent merger event resulting in a significant disturbance.

The dominant color is blue, suggesting ongoing star formation, particularly within the spiral arms and outer regions of the disk.