The galaxy presents a somewhat disturbed morphology, potentially indicating an interaction or merger event. It exhibits a disk-like structure, though its shape is irregular with some asymmetries. There is a noticeable central bulge with moderate luminosity. The overall color of the galaxy leans towards the redder end of the spectrum, suggesting an older stellar population, but regions of bluer light are also present, hinting at ongoing star formation. Patches of brighter emission are scattered throughout the galaxy, potentially indicating regions of active star formation. No strong spiral arm structures are immediately apparent. The light appears somewhat diffuse, giving it a "fluffy" look.
