The galaxy presents an irregular morphology. There is a slight central bulge, appearing diffuse rather than concentrated. This suggests it could be an irregular galaxy or a galaxy undergoing a merger. The dominant color appears to be red, potentially indicating a population of older stars. There is a hint of blue in some regions, which could indicate the presence of younger stars. Patches of possible dust lanes or obscured regions are interspersed. There is not a well defined disk structure. It shows signs of tidal tails or minor disturbances.
