The galaxy presents as a face-on spiral system. A bright, concentrated central bulge dominates the galaxy's core, exhibiting a yellowish-white hue suggestive of an older stellar population. Emanating from the bulge are loosely wound spiral arms, which appear somewhat fragmented and lack distinct definition. These arms display a bluer color compared to the central bulge, potentially indicating ongoing star formation. The overall morphology suggests a galaxy with a significant disk component, though the spiral structure is not highly pronounced. There may be some indications of minor disturbances to the structure, such as slightly asymmetric arm distribution, potentially suggestive of past interactions. The galaxy's light distribution is relatively smooth, with no prominent knots of star formation or distinct dust lanes clearly visible in this image.
