The galaxy presents a morphology indicative of a system undergoing, or having recently undergone, a significant interaction or merger. Two distinct nuclei are apparent, both exhibiting an orange-yellow hue suggestive of an older stellar population. The morphology is not clearly elliptical or spiral, with a disturbed structure and no apparent spiral arms. The overall appearance is relatively smooth. The light distribution appears centrally concentrated around each of the two nuclei, but the outer regions exhibit a more diffuse glow, potentially indicating tidal debris from the interaction. The color suggests this is a relatively massive galaxy with a low rate of star formation. Based on the visual evidence, the system is likely in a mid-stage of a merger event, or else a tidal encounter that has yet to settle into a regular configuration.
