The galaxy presents a generally smooth and elliptical morphology. It exhibits a high degree of central concentration, with the luminosity profile appearing more condensed toward the core. There is no discernible spiral arm structure or pronounced disk component visible in this image. The galaxy appears mostly round in shape. Some subtle color variations are present in the galaxy, particularly in the outer regions, which might suggest variations in stellar populations or dust content. There are no indications of significant tidal disturbances or ongoing major mergers based on the morphology. There might be some minor disturbance that can be observed but this is not certain.
