This galaxy appears to be a spiral galaxy exhibiting a notable disk structure. The arms are prominent, extending from a central bulge that is moderately sized in relation to the rest of the galaxy. There is evidence of a bar-like structure that extends from the central bulge through a significant portion of the galactic disk, but is not a particularly strong bar. The galaxy does not appear to be undergoing any major merging events, although a slight disturbance cannot be ruled out. The color indices suggest ongoing star formation. The estimated size of the galaxy is a diameter of roughly 6 kpc.
