The galaxy presents as a spiral, observed at a moderate redshift. The disk is not viewed edge-on, but at an angle allowing some structural details to be discerned. Prominent spiral arms are visible, loosely wound and extended, tracing outwards from a central bulge.

The bulge is significant, comprising a substantial portion of the galaxy's overall luminosity. A bar-like structure is subtly indicated near the center, possibly intersecting the bulge. The spiral arms exhibit flocculent features suggesting ongoing star formation, though no extremely bright, compact star-forming regions are readily apparent.

There is evidence of disturbance, potentially indicative of a minor interaction or merger event. This is characterized by asymmetry in the spiral arm structure. Overall, the galaxy appears to be a relatively luminous spiral galaxy with signs of recent or ongoing interactions influencing its morphology.
