The galaxy exhibits a well-defined spiral structure, presenting prominent arms. The central bulge appears relatively small to moderate in size, exhibiting a concentration of light. While there may be a bar structure in the center, this is difficult to say definitively.

There are regions of elevated star formation activity that stand out in the spiral arms, and an especially bright region on one edge.

The overall disk orientation seems to be closer to face-on than edge-on. The galaxy does not show any signs of major mergers.