The galaxy exhibits a relatively smooth, elliptical morphology. The central region displays a bright, concentrated core, suggesting a high density of stars. There is a disk-like structure to the outer regions. The color distribution appears to be fairly uniform across the galaxy, with the central region being slightly bluer. The outer regions, are also slightly bluer than the main body of the galaxy. The galaxy's shape is a well-defined elliptical. Evidence of disturbances are present, such as non-uniform density and a slight asymmetry of the edges. This suggests a possible interaction or merger history.
