The galaxy presents as a spiral type, with a disk-like morphology observed close to face-on. The spiral arms are clearly delineated, exhibiting a grand design structure. There appears to be two dominant arms that wind moderately tightly around the central bulge. The arms display a patchy distribution of light, suggestive of active star formation regions. The central bulge is noticeable, with what seems to be a concentration of older stellar populations, indicated by its orange hue. The overall color suggests a mixture of young, blue stars within the spiral arms and older, redder stars concentrated in the bulge. There is no strong evidence of a bar structure bisecting the bulge, but a subtle elongated structure cannot be ruled out. There is a minor asymmetry, possibly indicative of a recent or ongoing interaction or internal disturbance. The disk exhibits a relatively smooth texture with low granularity, consistent with a substantial red shift.
