The galaxy presents a predominantly disk-like morphology, although it exhibits both smooth and featured characteristics. A clear central bulge is observed, displaying a yellowish hue, suggestive of an older stellar population. The disk component shows a complex structure with areas that exhibit disturbances. While not an obvious major merger, there are indications of a minor interaction or disturbance, which are likely gravitational in nature. There is a blueish tinge to the outer edges of the disk, indicating younger stars in these regions. Overall the galaxy appears to be undergoing active, but moderate, star formation.
