This galaxy exhibits a relatively smooth, elliptical morphology. The core region appears intensely luminous, suggesting a high concentration of stars or potentially an active galactic nucleus. Moving outward from the core, the light gradually diminishes in intensity. There appears to be some disk structure to this galaxy. The color profile shifts from a warmer, yellowish-orange hue in the center to slightly cooler, greenish tones toward the periphery. It does not show any signs of major disturbances or mergers with another galaxy.
