The galaxy presents as a spiral type, with a clearly defined disk structure. The central bulge appears moderately prominent and exhibits a yellowish hue, suggesting an older stellar population. Faint spiral arms extend from the central bulge. Two dominant arms appear to wind outwards from the central area with a medium pitch angle. The arms exhibit a blue tint, possibly indicating areas of active star formation. There appears to be a bar feature, running through the center. The galaxy disk is not precisely edge-on, allowing some view of the spiral structure. The overall morphology indicates no obvious signs of recent major mergers, although some disturbance or interaction cannot be ruled out.
