The galaxy presents a largely smooth and rounded morphology. It appears elliptical in shape, with a highly concentrated central bulge that is bright yellow. Moving outwards from the center, there is a diffuse, less intense halo that presents some faint blue regions along the edges. Based on color, we see that there are likely some younger star forming regions in the outer halo. Overall, the image suggests a massive galaxy with a dominant old stellar population in the core, with ongoing star formation at a low rate. There is no evidence of a significant disk component or major merging events. It is experiencing at most minor disturbances.
