The galaxy exhibits a disk-like morphology, oriented at an oblique angle to our line of sight. It appears to be a spiral galaxy with a prominent bulge. The bulge dominates the central region, displaying a yellowish-white color, indicative of an older stellar population. The disk component shows bluer regions, particularly toward what appear to be the outer arms. This likely signifies regions of more recent and ongoing star formation. There appears to be a small amount of dust, perhaps obscuring some of the blue emissions. The disk of this galaxy is not uniform and may be disturbed or asymmetric. There also appears to be a significant amount of star formation happening throughout this galaxy. Overall, the galaxy appears to be a relatively massive spiral galaxy undergoing moderate star formation.
