The galaxy presents as a smooth, elliptical form, elongated in shape. The central region exhibits a bright, concentrated luminosity, possibly indicative of a dense stellar population or active galactic nucleus. Moving outward from the core, the light gradually diminishes, forming a diffuse halo. There is a subtle color gradient visible, with the central region appearing more yellow-red, potentially signifying older stellar populations, while the outer regions appear slightly bluer. The overall structure suggests a relatively evolved system, with minimal signs of recent major mergers or significant star formation activity. There's a slight asymmetry to the profile, hinting at a potential minor interaction or internal dynamic process.
