The galaxy exhibits a distinct spiral structure, characterized by two prominent, loosely wound arms. A stellar bar is visible across the central region, suggesting a barred spiral classification. A notable bulge is present, though not exceedingly dominant, exhibiting a moderate size relative to the galactic disk. Evidence suggests a dynamically active galaxy, undergoing some minor gravitational interaction or disturbance. The system displays varying degrees of star formation across its disk, with pockets of intense blue star formation regions. The overall color profile indicates a relatively young stellar population interspersed with older populations throughout the disk. The image is suggestive of a late-type spiral galaxy at moderate redshift.
