The galaxy presents a prominent disk structure with visible spiral arms. The arms appear relatively tightly wound around a central bulge. The bulge exhibits a yellowish hue, indicative of an older stellar population, while the spiral arms display a bluer color, suggesting ongoing star formation. The overall morphology suggests a classification towards the spiral type, but with a notable bulge component. There is no obvious sign of major interaction or merging events, although some minor asymmetry might be present within the disk.
