The galaxy appears to be a disturbed system, potentially undergoing a merger. There is evidence of tidal features. The central region presents a bright, somewhat amorphous core with diffuse light extending outwards. A faint, elongated structure can be seen extending from the core, suggesting a possible tidal tail. The system exhibits a blueish hue and a redder hue towards the edges indicating a possible change in the dominant stellar populations or dust content. The morphology suggests that the galaxy is not a pure elliptical or spiral, but rather a more complex, irregular shape.
