The galaxy appears as a relatively bright, flattened disk structure. It exhibits a smooth, centralized bulge that is more yellow in color compared to the rest of the disk. The disk itself shows hints of spiral arm structure, though these are not well-defined. The arms exhibit a bluer color compared to the bulge and the older inner regions of the disk, suggesting the presence of younger stellar populations. There is a faint asymmetry visible within the outer regions of the disk. This galaxy is a relatively isolated system, showing no major signs of a recent or ongoing major merger event, although minor disturbances cannot be ruled out. Overall, the system seems to be a relatively well-established and evolved spiral galaxy.
