The object appears to be a spiral galaxy, displaying prominent spiral arm structures. The arms are somewhat loosely wound and exhibit clumpy regions of star formation, suggested by the bluer hues in the arms. There is evidence of an ongoing merger event. One section of the galaxy appears to have been mostly distorted into a smooth section, while the other section retains more of its original structure. A bright central bulge is evident, contributing significantly to the galaxy's overall luminosity. There is not a strong central bar. The galaxy is oriented such that it's neither perfectly face-on nor edge-on, allowing for clear observation of both the disk and the bulge. The galaxy's apparent size suggests it is a moderately sized system, not exceptionally large or compact. Overall, the galaxy is a spiral type with signs of significant interaction and tidal disruption, indicative of a dynamic and evolving system.
