The galaxy presents as a face-on spiral, exhibiting a morphology characterized by prominent spiral arms. These arms display a mixture of medium and loose winding, suggesting differential rotation within the galactic disk. The central bulge is of moderate size relative to the disk, and shows very little smooth structure. The disk component dominates the galactic light profile. The galaxy is blue in coloration, indicative of active star formation, especially concentrated along the spiral arms. There seems to be a large amount of disturbance in the structure of the galaxy, indicating a potential major disturbance caused by a recent merger. Evidence of tidal features emanating from the main galactic body supports this interpretation, though these features are faint, suggesting a merger event in the past. No bar structure is clearly discernible in the image.
