This galaxy exhibits a disrupted morphology, possibly undergoing a merging event or tidal interaction. The main body of the galaxy appears elongated with hints of a distorted spiral or disk-like structure. There are some disturbances in the form of an outer tidal tail or bridge is visible, stretching away from the central region. The color is relatively blue in some regions and red in others, suggesting regions of active star formation mixed with populations of older stars. There appears to be distinct clumps of light, indicating possible regions of intense star formation or disrupted galactic nuclei. The lack of strong central concentration could be due to an ongoing merger. Overall, the galaxy is an interesting system showing signs of interaction and ongoing evolution.
