The galaxy exhibits a prominent spiral structure, characterized by two well-defined arms extending loosely from a central region. The spiral arms appear flocculent with regions of star formation and dust. The central bulge is moderately sized, and the core exhibits significant brightness. The overall disk appears face-on to the observer. The disk appears to be undergoing a major merger event. The galaxy exhibits a redshift, indicating it is at a significant cosmological distance. The galaxy displays characteristics indicative of an active star-forming environment, likely with a stellar mass near 10^10 solar masses.
