The galaxy presents a somewhat amorphous, rounded morphology. It is dominated by a smooth, diffuse central region exhibiting a yellowish-white hue, surrounded by less concentrated halos of orange and red. There are no clear spiral arm structures or a distinct galactic bar visible. The color gradients suggest variations in stellar populations and dust content across the galaxy, but the poor resolution makes it difficult to be certain. The color indices suggest relatively evolved stellar populations. The overall appearance suggests a massive system, potentially an elliptical galaxy or a spiral undergoing a merger. There seems to be an interaction, or perhaps a merger event between multiple galactic structures in progress.
