The galaxy presents as a relatively smooth, elliptical-like structure. The central region exhibits a high concentration of light, indicative of a prominent galactic nucleus. The light gradually diffuses outwards from the core, with no distinct spiral arm structures visible. There is some subtle evidence of a disk, but it is not sharply defined. The color profile suggests a population of older stars, with a general lack of prominent blue regions that would otherwise indicate active star formation. Some minor disturbances could potentially be present, but they are not strongly apparent.
