The galaxy presents as a spiral type, exhibiting well-defined arms. The arms appear tightly wound around a central bulge. The central bulge is small relative to the overall disk size. The disk component is dominant. The color of the central region appears slightly more yellow/white, suggesting an older stellar population compared to the bluer arms, which implies ongoing star formation. The spiral arms are fairly symmetrical. There is no apparent major disturbance or signs of a major ongoing merger. There is no strong bar structure visible, though a weak bar presence cannot be ruled out. The galaxy is viewed from a predominantly face-on orientation, and is relatively isolated.
