The galaxy presents as a spiral morphology. Its nucleus exhibits a concentrated luminosity, indicative of a likely supermassive black hole.

The disk is not viewed edge-on, but rather at a more inclined angle, allowing for the discernment of spiral arm structure. The arms themselves are tightly wound around the central bulge. The disk contains noticeable star-forming regions.

Overall, the structure suggests a spiral galaxy that is currently evolving with moderate star formation activity, and no evidence of significant interaction with another galaxy.
