The galaxy presents a largely smooth and somewhat elliptical morphology. The color profile suggests a dominant population of older stars, likely in the bulge region, indicated by the central yellowish-white hue. There is evidence of a faint disk-like structure surrounding this core, exhibiting a bluish tint, hinting at the presence of younger, hotter stars.

The galaxy appears relatively undisturbed, showing no significant signs of ongoing major mergers. However, a hint of asymmetry in the outer regions might suggest minor gravitational interactions or past minor mergers. Overall, this appears to be a galaxy in a relatively advanced stage of evolution, with ongoing but likely subdued star formation activity.
