The galaxy presents a generally smooth morphology, appearing somewhat rounded in shape. There is a central concentration of light, surrounded by a more diffuse and extended halo or disk. Faint features suggest subtle disturbances or possibly spiral arm structures, although these are not strongly defined. The galaxy exhibits a color gradient, appearing bluer toward the center and redder in the outer regions. This may indicate younger stellar populations in the central region, and older stellar populations in the outer regions. There are no obvious signs of a major ongoing merger, however, close inspection suggests a minor disturbance, potentially caused by a previous interaction. The overall color of the object indicates it has an intermediate redshift, although no exact value can be determined from a visual inspection of a still image.
