The galaxy exhibits a prominent spiral structure. Two well-defined spiral arms emanate from a central bulge, displaying a relatively loose winding pattern. The disk component appears to be the dominant feature, with the spiral arms contributing significantly to the overall luminosity. The bulge appears to be of moderate size in relation to the disk.

The arms display a mottled texture, indicative of active star formation regions. No clear evidence of a strong central bar is visible; a weak bar may be present but difficult to resolve. The galaxy shows signs of mild interaction or disturbance.
