The galaxy presents as a spiral type, displaying a prominent disk structure. Spiral arms are visible, although the resolution limits a detailed assessment of their morphology. The galaxy exhibits a central bulge of moderate size. There may be a weak bar-like feature spanning the central region. No major signs of ongoing or recent merger activity are visible. A significant portion of the light appears to be originating from star formation within the disk. The edge-on inclination of the galaxy is relatively low, allowing for a face-on view of the spiral structure.
