The galaxy appears to be a relatively smooth, elliptical galaxy at a considerable distance, as evidenced by its small angular size. The central bulge exhibits a bright, concentrated luminosity gradient, indicative of a high stellar density. Moving outwards from the core, the luminosity gradually decreases, transitioning into a fainter, more diffuse halo. There is a subtle color gradient observed, with the central region appearing slightly yellower than the outer regions, possibly suggesting a population of older, redder stars concentrated toward the center. I see no obvious spiral arm structure or dust lanes within the galaxy. There are no obvious signs of strong tidal interactions or major ongoing merger events, though slight morphological disturbances can't be ruled out at this resolution. The galaxy's overall shape appears approximately round.
