The galaxy presents a predominantly smooth morphology, with a high degree of central concentration. It appears elliptical in shape, though with some slight elongation suggestive of a flattened spheroid. The central region exhibits a bright, yellowish-white core, which fades into a less luminous, more diffuse halo with hints of blue. There is no readily apparent spiral structure or distinct dust lanes within the galaxy. Overall, it presents the characteristics of an evolved system with a significant population of older stars. There does not appear to be any indications of merging or major disturbances in its structure.
