The galaxy appears as a concentrated, elliptical-like structure. Its core exhibits a prominent, bright, yellowish-white glow, suggesting a significant concentration of older stars and possibly a supermassive black hole actively accreting material. The galaxy's overall shape is smooth and regular, lacking any distinct spiral arms or irregular features. The color gradient transitions from a yellowish-white center to a more orange hue as it expands to its full extent. The outer regions appear faint and ill-defined, indicating a gradual decrease in stellar density with an absence of ongoing, significant star formation, corresponding with its small specific star formation rate. There is no apparent evidence of tidal disturbances or ongoing mergers with other galaxies. The overall impression is that of a large, evolved system.
