The galaxy appears as a centrally concentrated system, likely an elliptical galaxy given its smooth morphology. The core region exhibits a yellowish hue, which may indicate an older stellar population. The surrounding halo displays a slight radial color gradient, transitioning to a bluer shade further from the core. There is no visible structure such as spiral arms or a prominent disk. The overall shape seems relatively round, with some minor deviation from perfect circularity. No signs of any major disturbances or merging events are directly visible, but subtle asymmetries cannot be ruled out due to the galaxy's distance. The galaxy appears relatively quiescent, with a low rate of recent star formation, consistent with the aged stellar population inferred from its color.
