The galaxy presents a prominent disk structure, exhibiting well-defined spiral arms. These arms appear tightly wound, suggesting a relatively high rate of shear in the disk. The central bulge is small relative to the size of the disk, indicating a disk-dominated morphology. There is no obvious bar structure visible in the central region. The color distribution suggests the presence of ongoing star formation activity, particularly within the spiral arms, as evidenced by their bluer hue. The galaxy does not appear to be undergoing a major merger event, although a possible minor interaction is suggested by slight asymmetries in the outer disk regions. The overall morphology is consistent with that of a late-type spiral galaxy.
