The galaxy presents as a roughly elliptical structure with a smooth overall appearance. The core region exhibits a concentrated, brighter emission, suggesting a higher density of stars in that area. Moving outwards from the core, the light gradually diffuses, indicating a decreasing stellar density. There is a hint of what might be spiral arm structures but that is not clear. The galaxy's color profile suggests a population of older stars, potentially with a lower rate of active star formation. Some minor disturbances are present in its shape, but it shows no obvious signs of a major ongoing merger event. The lack of prominent dust lanes or patchy regions further supports a relatively quiescent state.
