The galaxy presents as a complex system, exhibiting features indicative of a possible ongoing interaction or merger. Two primary luminous regions are observed. The upper region appears smoother and more centrally concentrated, with a yellow-orange hue, suggesting an older stellar population. A distinct bridge of material connects this region to a lower, bluer region. This connecting feature is less regular and more extended, implying tidal forces may be at play. The lower region is bluer, indicating the presence of younger stars and potentially active star formation.

The overall shape is not clearly elliptical or spiral, appearing somewhat irregular. This morphological disruption supports the hypothesis of an interaction. The light distribution suggests a significant fraction of the light comes from a relatively smooth component but is marked by the presence of disturbed regions. There is no clear single nucleus. The system is moderately luminous, inferring a substantial stellar mass. The color indices imply it lies at a considerable distance, as confirmed by its estimated redshift. The very low specific star formation rate suggests that, although there are areas of younger stars, the star formation is not very active compared to the overall mass.
