The galaxy presents as a spiral galaxy, exhibiting prominent spiral arm structure. A moderate bulge is visible at the galaxy's center, displaying a yellowish hue, indicative of an older stellar population. The spiral arms appear relatively flocculent and loosely wound. The disk displays a bluish tint, suggesting ongoing star formation. There is some evidence of possible tidal disruption or interaction based on asymmetry in the disk. There are several star forming regions visible along the spiral arms. The color bands show star formation is relatively moderate. Overall, the morphology suggests a disk galaxy with spiral arms and a moderate central bulge, currently undergoing active star formation.
