The galaxy presents as a well-defined spiral structure. Two prominent spiral arms are visible, extending outwards from a central bulge region. The arms are delineated by a mottled texture indicating regions of star formation. There appears to be a slight hint of a bar-like feature across the bulge, though it is not a dominant structure. The bulge itself appears relatively moderate in size. The winding of the spiral arms seems to be somewhere between tight and medium. There is no indication of a major merging event but what appears to be a minor disturbance.
