The galaxy presents as a relatively bright, face-on spiral. A discernible central bulge is apparent, though not overly prominent, with a moderate size in relation to the overall galactic disk. The spiral arms appear tightly wound around the central bulge, displaying a multi-armed structure that is difficult to definitively resolve, however, it appears there are two or three dominant arms. The color gradient suggests active star formation. There appears to be some minor disturbance or asymmetry in the outer regions of the disk, hinting at a potential interaction.
