The galaxy appears as a flattened, elliptical shape, suggesting a disk-like structure viewed nearly edge-on. There's a noticeable central bulge that appears brighter and more concentrated than the surrounding regions. The color gradient transitions from a yellowish-white core to bluish hues at the outer edges of the disk. The disk shows limited discernible spiral arm structure, appearing relatively smooth with subtle variations in brightness. The light distribution suggests ongoing, though not vigorous, star formation activity. The overall morphology indicates a relatively high probability of being an edge-on disk galaxy with a considerable stellar mass. There does not appear to be a merger occurring, although there may be some minor gravitational disturbance given the subtle asymmetry in the disk.
