The galaxy presents as a spiral type, observed at an angle close to face-on. A central bulge is apparent, exhibiting a yellowish hue, possibly indicating an older stellar population. The disk shows a distinct spiral arm structure. Two prominent arms can be traced from the central region, characterized by a bluer color suggesting ongoing star formation. The spiral arms appear somewhat fragmented and uneven. A faint bar structure may be present across the central bulge region. No significant signs of major mergers are apparent, though there might be some minor asymmetry in the arm structure. The central bulge appears moderately sized compared to the overall disk. The spiral arms are moderately wound.
