The galaxy presents as a spiral type, viewed at an angle that is neither edge-on nor face-on. Definite spiral arms are apparent, although the exact count is difficult to discern due to their patchy and somewhat indistinct nature. The winding of these spiral arms appears relatively tight in some regions and more open in others, creating a somewhat irregular appearance.

A central bulge is present but does not dominate the overall structure. No obvious bar feature is immediately apparent. 

There is evidence of interaction or disturbance, possibly a minor disturbance. The spiral arms appear somewhat disrupted and asymmetric, potentially suggesting an ongoing or recent merger event. Patches of blue light indicate regions of active star formation.
