The object appears to be a spiral galaxy, observed at an angle approaching edge-on. There is evidence of a galactic bulge, appearing as a central concentration of light, slightly brighter than the surrounding disk. The disk itself appears relatively thin and elongated.

The galaxy exhibits a subtle colour gradient, transitioning from a more blue hue at the edges of the disk to a slightly redder colour toward the central bulge. This could imply younger stellar populations towards the outer regions, and older populations concentrated in the bulge.

There seems to be some disturbance in the disk's shape; it may be asymmetrical, potentially due to past gravitational interactions or a minor merger event. The shape isn't a smooth ellipse, and there may be an arm or other stellar structure being pulled away from the main disk, although this is not certain.

The overall morphology suggests a complex formation history or ongoing interaction with another galaxy or intergalactic medium. Further spectroscopic analysis would be valuable in determining the galaxy's redshift, stellar populations, and any active galactic nucleus activity.
