The galaxy presents a complex morphology, suggestive of a spiral structure, although disturbed. A prominent central bulge is observed, exhibiting a yellowish hue, possibly indicating an older stellar population. Fainter, bluer regions are visible outside of the main central bulge. There is evidence of multiple spiral arms extending outwards, some tightly wound. The arm structure appears flocculent and somewhat asymmetrical, with the winding being relatively tight in a number of arms. The disk shows a slight inclination. The arms are very faint, and are more easily discernable at the bottom of the galaxy than the top. There is a noticeable dust lane or obscuration within the disk structure. Possible merging or tidal features are visible.
