The galaxy presents as a spiral type, with prominent, well-defined spiral arms extending from a central bulge. The arms exhibit a moderate degree of winding, neither tightly wound nor completely open, and appear to trace out a grand design. The number of spiral arms is predominantly two, although some arms may bifurcate.

The central bulge appears moderately sized relative to the disk. No obvious bar structure bisects the bulge.

The galaxy's disk shows indications of ongoing star formation. No obvious major merging events, but minor disturbances may be present. The galaxy's overall structure is dominated by the disk component.
