The galaxy exhibits a complex morphology, appearing to be in the late stages of a merger event. The primary galaxy displays an elliptical shape with a high degree of central concentration. A secondary, smaller component is observed on the periphery. The presence of tidal tails or other obvious signs of disruption is minimal, suggesting that the interaction is well advanced. The color gradient is relatively smooth across the galaxy, with a slight reddening towards the core, and a blueish hue in areas of what might be star formation. The overall structure indicates a relatively evolved system, potentially evolving into a more spherical morphology.
