The galaxy presents as a spiral galaxy with a prominent disk. The disk shows a slight tilt relative to our line of sight. Two distinct spiral arms are visible, extending from a moderately sized central bulge. These arms appear tightly wound. The central bulge is yellowish-white, potentially indicating an older stellar population. The arms are bluer in color, suggesting ongoing star formation. There appears to be a bar-like structure within the bulge. The galaxy shows no obvious signs of major mergers, but there may be some indication of minor disturbances in the disk structure. The outer regions of the galaxy fade into a fainter halo.
