This galaxy appears to be undergoing a significant interaction or merger. The morphology is complex and disturbed, with an irregular shape that deviates substantially from a smooth elliptical or spiral structure. There is a bright, central region that is elongated, with a secondary bright region distinct and separate from the core, suggesting the presence of multiple galactic nuclei or intense star-forming regions associated with tidal tails. The object exhibits a faint, diffuse halo that is not uniform. The object exhibits a blue hue, indicating a younger stellar population. This suggests the presence of active star formation.

The overall impression is that of a dynamic system undergoing gravitational interactions, possibly a merger between two or more galaxies. The morphology suggests a system far from equilibrium.
