The galaxy appears to be a relatively smooth, elliptical galaxy with a bright, concentrated central bulge. The light from the galaxy is centrally concentrated, with a noticeable decrease in surface brightness moving outwards. The central region exhibits a yellowish hue, potentially indicating an older stellar population, while the outer regions show a faint bluish tint, possibly suggesting a small amount of recent star formation. There is no evidence of spiral arms, bar structures, or significant dust lanes. The galaxy appears largely undisturbed, with no signs of major mergers or tidal distortions. The overall morphology indicates a system that is likely dominated by an evolved stellar population, with a smooth, round appearance.
