The galaxy presents as a merging system, with two distinct, luminous nuclei indicative of two interacting galaxies. The overall morphology suggests a state of late-stage merger, with a significant amount of tidal distortion apparent. The color profile appears complex, with a central yellowish-white hue surrounded by diffuse regions of redder emission. This suggests a mix of stellar populations with potentially ongoing star formation. The angular size of the galaxy appears relatively compact, though the presence of tidal features suggests that it may be more spatially extended than initially apparent. The overall appearance supports classification as an interacting system undergoing a major merger event.
