The galaxy presents as a dual-core system, suggesting an ongoing or recent merger event. The primary core exhibits a smoother, more diffuse morphology with a yellowish-white hue, indicative of an older stellar population. The secondary core is more compact and displays a distinct orange color, possibly indicating ongoing star formation or a dust-reddened population. There are slight irregularities in the overall shape, likely due to gravitational interactions. Weak tidal features might be present, although low image resolution limits definitive assessment.
