The galaxy presents a generally smooth and elliptical morphology, with a high degree of central concentration. The light distribution appears relatively symmetrical. The visible color gradient suggests a bluer inner region, transitioning to redder outer regions, which could indicate differential stellar populations, with younger, hotter stars more concentrated towards the center and older, cooler stars dominating the outskirts. There is little to no apparent dust or prominent spiral arm structure within the galaxy. Overall, the galaxy appears as a well-formed elliptical galaxy at a moderate redshift, with a significant stellar mass.
