This galaxy exhibits a complex morphology, showing characteristics of both a smooth and a disk-like structure. The central region is bright, exhibiting a high degree of luminosity, potentially indicative of an active galactic nucleus or a region of intense star formation. The overall color of the galaxy appears to be shifted towards the red end of the spectrum. There is evidence of a possible ongoing interaction or merger with a smaller companion galaxy. The disk component shows faint spiral arms. The overall mass of the galaxy appears to be considerable, with evidence of ongoing star formation.
