The observed galaxy presents as a face-on spiral structure, exhibiting a prominent central bulge. The bulge appears moderately sized and intensely bright, possibly indicating a supermassive black hole and active galactic nucleus at the center. Spiral arms are clearly visible, emanating from the central bulge. The winding of these arms appears mostly tight but some areas are slightly looser. There are at least 4 spiral arms. There is no apparent bar structure. The disk is the dominant feature. The overall color of the galaxy appears to be dominated by blue hues, potentially indicative of active star formation. There is no major disturbance or merger happening, though some minor disturbances could be present, though that could be artifacts of the image.
