The galaxy presents an irregular morphology. Its light profile is diffuse, with a brighter, seemingly smooth central region that fades into a less defined extended halo. There is evidence of possible tidal tails or streams emanating from the main body, suggesting gravitational interaction with another object or a past merger event. The overall color appears bluish, potentially indicative of recent star formation activity, although reddening could be present due to dust. There are some areas that are more clumpy in appearance.
