The galaxy presents a generally smooth, elliptical morphology. A bright, concentrated central bulge dominates the structure, exhibiting a yellow-white hue. This suggests a population of older stars within the core. Progressing outwards, the color subtly transitions to a greenish-blue, possibly indicating regions of ongoing, though not prolific, star formation within a disk-like structure. The galaxy appears relatively undisturbed, with no obvious signs of recent major mergers or tidal interactions. Overall, the light distribution is quite symmetric and concentrated, consistent with an early-type galaxy at a moderate redshift.
