The galaxy presents as a spiral galaxy with a clearly defined disk structure. The spiral arms exhibit a tightly wound morphology, with multiple arms emanating from the central region. A bulge is visible, but appears relatively small in comparison to the disk. The galaxy displays a blue hue, suggesting a significant population of young, hot stars and active star formation. While the overall structure appears largely undisturbed, some minor asymmetries are present in the outer regions of the disk, hinting at a potential interaction or disturbance. There may be a slight indication of a bar structure present in the central region, but this requires higher resolution imaging for confirmation.
