The galaxy presents as a disk-shaped structure with an overall elliptical morphology. Its central bulge appears bright and yellowish-white, indicating an older stellar population. The disk component shows a color gradient, transitioning from a bluer hue in the outer regions to a more yellow-red color closer to the center. There appears to be a slight asymmetry or minor disturbance visible in the outer regions of the disk, though the overall structure does not indicate a major ongoing merger event. The smoothness of light distribution suggests that a significant portion of the galaxy's light is due to a smooth stellar distribution. The galaxy shows signs of ongoing, moderate star formation activity. The overall impression is of a relatively massive galaxy at a moderate redshift.
