The galaxy presents as an elongated, elliptical morphology. The core region exhibits a concentrated, bright glow indicative of older stellar populations. Moving outward from the center, the luminosity gradually diminishes, and the color appears slightly bluer and more muted. There is no evidence of strong spiral arm structures or active galactic nuclei activity discernible within this image. Minor disturbances are possibly occurring. Overall, the galaxy appears to be a large, relatively old system with a low ongoing star formation rate.
