The galaxy presents a relatively face-on orientation with a disk structure exhibiting prominent spiral arms. The arms are fairly tightly wound, appearing almost flocculent in nature, extending outward from a moderately sized central bulge. The bulge shows a smooth distribution of light. The overall color of the disk appears blue, suggesting ongoing star formation, with the inner regions displaying a slightly redder hue indicative of older stellar populations. The morphology suggests a well-defined spiral structure. There are hints of disturbances in the galaxy's structure, which may suggest a possible interaction or merger history.
