The galaxy presents a largely smooth morphology, with a slightly flattened, elliptical appearance. The light distribution is centrally concentrated, exhibiting a gradual decrease in intensity outward from the core. There is a distinct color gradient, with the central region appearing more reddish, transitioning to a more greenish-bluish hue in the outer regions. The overall structure indicates a relatively evolved system with a well-established stellar population. While the image doesn't reveal any prominent spiral arms or distinct dust lanes, there are hints of subtle, diffuse features that might suggest underlying structural components or recent star formation activity in the outer regions. There is no clear indication of ongoing major mergers or significant tidal disturbances.
