The galaxy appears to be a spiral type, exhibiting prominent spiral arm structures. These arms are well-defined and extend outwards from the galactic center. The galaxy is not perfectly symmetrical.

Evidence of star formation is visible within the spiral arms, with regions of intense activity indicated by a change in color. A central bulge is present, though it appears to be of moderate size compared to the overall galactic disk.

The disk is inclined relative to our line of sight, as opposed to appearing directly face-on. There is potential evidence of a bar-like structure crossing the central region of the galaxy.

Finally, the outer regions of the galaxy show indications of interaction or disturbance, possibly a merger.
