The galaxy presents a generally smooth, elliptical morphology, with a high degree of central concentration. The core region exhibits a bright, luminous appearance, suggesting a significant population of stars. Moving outwards from the core, the light gradually diminishes. There is a very faint blue color in the outer regions which could indicate areas of low level star formation or remnants of a disk. The overall rounded shape is without any obvious distortions or signs of ongoing major mergers. Any activity appears settled or minimal.
