The galaxy presents as a somewhat disturbed disk galaxy, with a prominent central bulge that is slightly offset from the main disk. There is evidence of ongoing star formation within the disk, particularly noticeable as brighter blue regions. The overall structure appears asymmetric, possibly indicating a recent interaction or merger event. The dust lanes appear to be relatively faint and diffuse. The galaxy exhibits a slight elongation, and the disk has a moderate inclination relative to our line of sight. There appears to be a tidal tail or stream of material extending from one side of the disk, further suggesting gravitational interaction.
