The galaxy exhibits a complex morphology, with features indicating both spiral structure and potential interaction or merging. The central region displays a moderate bulge component. Prominent spiral arms emanate from this central region, exhibiting a loosely wound structure and extending outwards. These arms show clear evidence of active star formation, highlighted by the presence of bright, blue-ish knots indicative of young, hot stars. There seems to be a weak bar-like structure within the central region, though it does not appear to be strongly defined. The overall color of the galaxy suggests a mix of stellar populations, with regions of both young, blue stars and older, redder stars. The disk is oriented closer to a face-on perspective. There is possible evidence of a merging event or minor disturbance.
