The galaxy appears as a relatively smooth, elliptical-like object with a centrally concentrated light profile. The core region displays a yellowish hue, suggesting an older stellar population dominates in this area. A gradual decline in color and luminosity is observed moving outward from the core, transitioning to a bluer tint in the outer regions. There is little to no apparent spiral arm structure or dust lane obscuration visible in this image. The overall morphology indicates a system that is well-evolved, with no indication of major merger events or significant tidal disturbances.
