The galaxy presents a prominent disk structure, with definitive spiral arm morphology. Two distinct spiral arms are clearly visible, emanating from a central bulge. The arms exhibit a medium winding pattern and appear somewhat flocculent. The central bulge appears moderately sized. A possible bar feature is present, and may be considered strong. Overall, the galaxy displays a classic spiral structure with moderate star formation occurring in the disk. There is no evidence of significant tidal disruption or ongoing major merger activity.
