The galaxy presents as a face-on spiral with a prominent central bulge exhibiting a yellowish-white hue, potentially indicative of an older stellar population. The spiral arms appear well-defined but somewhat tightly wound, exhibiting a distinct bluish tint suggestive of ongoing star formation. The disk is not perfectly circular, showing a slight elongation. Some irregular features are present within the spiral arms, possibly regions of enhanced star formation or dust obscuration. There is a faint suggestion of a bar-like structure across the central region. No obvious signs of a major ongoing merger are apparent, although some minor disturbances in the arm structure cannot be ruled out. The galaxy exhibits moderate luminosity, displaying a size consistent with a typical spiral galaxy at its redshift.
