The observed galaxy exhibits characteristics indicative of an ongoing or recent merger event. The light profile suggests two distinct, yet interacting, galactic nuclei within a common envelope. The overall morphology is disturbed, lacking the defined spiral arms or elliptical structure typical of undisturbed galaxies. The system is dominated by smooth light, with little evidence of distinct dust lanes or knotty star-forming regions. The color suggests an older stellar population, implying that the majority of star formation occurred in the past. The object is roughly circular, with a slight elongation along the axis connecting the two nuclei. The observed features point to a system with high luminosity and a significant mass.
