The galaxy presents a distinct spiral structure. The arms appear tightly wound around a central bulge, which has a moderate size relative to the overall galactic disk. The spiral arms themselves are prominent, with a notable presence in the galaxy. The galaxy appears to be relatively undisturbed, showing no signs of ongoing major merging events, although some minor disturbances may be present. Star formation appears to be low to moderate, with a blueish hue indicating areas of possible recent star formation. A weak bar structure may be present.
