The galaxy appears to be a spiral galaxy, viewed at a near edge-on angle, showing a prominent disk. Within the disk, spiral arm structures are faintly visible, with a tightly wound appearance. The central bulge region is noticeable, exhibiting a moderate size relative to the overall disk. The galaxy displays a bar-like feature extending through the center.

There seems to be a strong indication of substantial star formation activity within the galaxy, as evidenced by the vibrant light emitted. The disk also has signs of minor disturbances, possibly indicative of gravitational interactions or recent mergers.

The morphology suggests an evolving system with a mixture of old and new stellar populations.
