The galaxy presents an overall elliptical morphology, exhibiting a smooth, relatively featureless light distribution. The central region displays a higher concentration of light, appearing brighter and more compact. There is a gradual decrease in surface brightness as one moves outward from the center, with no obvious spiral arm structures visible.

The galaxy exhibits a subtle color gradient, with the central region appearing slightly redder in comparison to the bluer outer regions. This suggests a difference in stellar populations, with older, redder stars dominating the core, and younger, bluer stars populating the outer areas. The galaxy shows hints of disturbance. Further observations are needed to determine the full extent of any interactions.

Given the overall shape and color characteristics, this galaxy is likely an elliptical galaxy at a moderate redshift.
