The galaxy presents an elongated morphology, suggestive of a disk-like structure viewed at a significant angle. The central bulge region exhibits a yellowish hue, potentially indicating an older stellar population. Moving outward from the center, the disk displays a subtle bluer coloration along its edges, hinting at ongoing star formation within the spiral arms. The galaxy appears relatively smooth, but subtle irregularities or disturbances exist within the structure that hint at a past or ongoing interaction. Based on its color, the amount of new stars being formed appears to be relatively low. 