The observed galaxy exhibits a morphology indicative of a spiral structure, though the resolution limits detailed characterization. Two prominent spiral arms are clearly visible, loosely winding around the central bulge. The bulge appears moderate in size compared to the overall galactic disk. A slight asymmetry in the spiral arm distribution suggests possible gravitational interaction or past merging event. There appears to be a companion object interacting with this galaxy on the right, this could also be the result of a major disturbance or merger within the galaxy itself. The disk component appears to be the dominant feature of the galaxy. Star formation is likely occurring.
