The galaxy presents as a relatively smooth, centralized object. Its morphology appears predominantly elliptical, with a high degree of roundness, showing little to no disk-like structure or spiral arms visible in this image. The core of the galaxy exhibits a bright, concentrated luminosity, which gradually fades towards its outer regions. Color gradients are subtle, suggesting a relatively homogenous stellar population. The galaxy shows no obvious signs of major mergers or significant disturbances in its overall structure. There are hints of a green hue around the core suggesting some star formation, but generally it looks like an older galaxy.
