The galaxy appears to be a relatively smooth, elliptical morphology. The light is concentrated towards the center, indicating a prominent galactic bulge. The shape is largely circular, with only a minor deviation from perfect roundness. There is no clear indication of a disk component or spiral arms, nor are there any signs of any major mergers or disturbances. There is a slight color gradient, with the central region appearing somewhat bluer than the outer regions. The relatively smooth profile and color suggests a population of older stars, although there may be some ongoing star formation present, especially in the core.
