The galaxy appears to exhibit a disturbed morphology, possibly indicative of an ongoing or recent interaction. There is a faint blue hue evident, suggesting the presence of younger stellar populations and ongoing star formation. The galaxy does not possess a well-defined, smooth structure, but rather appears clumpy and irregular. A tidal tail or bridge feature appears to be present, further supporting the notion of gravitational interaction. A significant amount of the light appears to be concentrated in a central region, although the core is not particularly bright or point-like. Overall, the galaxy seems to be in a state of dynamic evolution due to internal or external processes.
