The galaxy displays a complex morphology, potentially indicating an interaction or merger event. It presents two distinct luminosity concentrations. The larger, more prominent concentration appears spheroidal, exhibiting a smooth light distribution with a yellowish hue, suggestive of an older stellar population and a lack of significant ongoing star formation in its core. A fainter, disk-like structure extends away from this central bulge. This disk exhibits a more irregular and clumpy appearance, with a reddish-orange color, which indicates the possibility of dust obscuration and potential star formation regions. There is evidence of some disruption in the overall structure, potentially in the form of tidal tails or asymmetries in the disk. The overall color suggests a population of relatively old stars. 
