The observed galaxy presents a distinct spiral structure, though the orientation is not perfectly face-on. The spiral arms are clearly delineated and show moderate winding, appearing somewhat tightly wound in some regions and more loosely wound in others. Two primary spiral arms appear to dominate the structure, although several more less prominent arms seem present.

The central bulge region exhibits a yellowish hue, suggesting an older stellar population. The disk of the galaxy shows variations in color, with bluer regions indicative of ongoing star formation. The dust lanes are subtly visible along the inner edges of the spiral arms, contributing to the contrast and definition of the spiral structure.

The galaxy appears to be relatively undisturbed, without major signs of ongoing or recent merger activity. The overall symmetry and well-defined spiral arms suggest a dynamically evolved system. 
