The galaxy exhibits a clear spiral structure, with a high probability of spiral arms being present. The arms appear somewhat tightly wound. There may be two dominant arms, with some ambiguity. A central bulge is observed, but it is not particularly dominant compared to the overall size of the galaxy. There is a possible indication of a weak bar-like structure across the central region, though it is not clearly defined. No strong signs of ongoing major merger activity are apparent, though subtle disturbances cannot be ruled out. The galaxy appears moderately luminous.
