The galaxy presents as a relatively smooth, elliptical-like structure. The core exhibits a concentrated, bright yellowish-orange hue, indicating a likely concentration of older stars. The outer regions display a gradual decrease in luminosity, fading into the background sky. There's a subtle color gradient from the core outwards, with the outer regions showing hints of redder tones, but no distinct spiral arms or significant dust lanes are apparent. The galaxy appears largely undisturbed with no indications of a major merger in progress, although the possibility of a minor interaction cannot be ruled out based on this image alone. The overall morphology suggests an evolved system dominated by an older stellar population and a relatively low rate of star formation.
