The galaxy presents a disturbed morphology, showing evidence of possible interaction or tidal disruption. The central region exhibits a somewhat diffuse, elongated structure with hints of a brighter core. Faint extensions or tails are visible, suggesting ongoing gravitational interactions. A prominent, slightly curved arm extends outwards from the main body. Color variations across the galaxy are noticeable, with bluer regions possibly indicating areas of active star formation and redder areas indicative of older stellar populations. Overall, the galaxy appears to be in a dynamic state.
