The galaxy presents as a relatively smooth, elliptical structure. Its color profile appears to be somewhat redder in the central regions, transitioning to a bluer hue towards the outer edges, possibly indicating differing stellar populations or dust distribution within the galaxy. The galaxy appears to be well-defined, exhibiting a moderate degree of roundness, without any strong visible features such as spiral arms or significant irregularities. There does not appear to be any on going or past merging activity.
