The galaxy appears to be a relatively smooth and concentrated elliptical galaxy, with a high degree of central symmetry. The light profile suggests a central bulge of older stars. The shape is generally round, though with some elongation. There are no clear signs of spiral arms or significant dust lanes visible in the image. The galaxy exhibits a concentrated, luminous core. There are hints of faint features in the outskirts, suggesting the presence of a diffuse stellar halo surrounding the main body of the galaxy. It is likely not a merger based on the smooth features and a lack of strong tidal tails.
