This galaxy exhibits a distinct spiral structure. Two prominent spiral arms extend from the central bulge, exhibiting a loose winding pattern. The galaxy presents a somewhat flocculent appearance, with the spiral arms not entirely continuous or well-defined. The bulge appears to be of moderate size relative to the overall galactic disk. There is no obvious presence of a strong central bar. The overall orientation suggests a face-on view. Evidence of ongoing star formation is suggested by the mottled texture of the spiral arms and the presence of some areas exhibiting a bluer hue. There is no immediately apparent evidence of a major ongoing merger, although minor disturbances cannot be ruled out. The color suggests an intermediate redshift.