The galaxy presents a clear spiral morphology with two distinct arms. These spiral arms exhibit a medium winding pattern, extending outwards from a central bulge. The bulge appears relatively small and somewhat indistinct from the surrounding disk. A bar-like structure is present traversing the central region, although it is not prominently defined. The disk of the galaxy is oriented face-on relative to our line of sight. There is no major interaction or merging events are apparent, though there is some indication of minor disturbance in the galaxy's form. The spiral arms are of an even colour, suggesting even rates of star formation throughout.
