The galaxy presents as a spiral galaxy, observed face-on. There is a prominent central bulge exhibiting a yellow hue, suggestive of an older stellar population. The spiral arms, though not sharply defined, are readily discernible and appear to wind moderately tightly around the central bulge. The arms display a bluer color, indicating the presence of younger, hotter stars and active star formation regions. The disk exhibits a degree of patchiness, possibly indicating regions of varying stellar density or dust obscuration. The galaxy doesn't appear to be strongly barred. No major signs of interaction or recent merger events are readily apparent, although some minor irregularities may be present within the arms. The overall morphology suggests a galaxy with ongoing star formation within its spiral arms and a significant, relatively evolved bulge component.
