The observed galaxy exhibits a clear spiral structure, although the resolution limits precise tracing of individual arms. The arms appear relatively tightly wound. A central bulge is visible and appears of moderate size, exhibiting a yellowish hue, suggesting a population of older stars. The disk component of the galaxy is prominent, showcasing a bluer coloration which likely indicates ongoing star formation within the spiral arms. The galaxy's orientation presents it as somewhat edge-on from our perspective. The overall shape indicates the galaxy is neither perfectly face-on nor perfectly edge-on, allowing us to discern both the spiral structure and a sense of the disk's thickness. There is no immediately apparent evidence of a major ongoing merger, although some minor asymmetries in the disk's light distribution hint at possible past interactions or internal disturbances. A subtle bar structure may be present, though it is not a particularly strong or well-defined feature.
