The galaxy presents as a relatively smooth, centrally concentrated structure with an elliptical morphology. The core region exhibits a bright, yellowish hue, suggesting a population of older, evolved stars. Extending outward from the core, a fainter, diffuse halo of bluish light can be observed. The blue color indicates the presence of younger, hotter stars, suggesting some ongoing, albeit low-level, star formation. There are no obvious signs of strong spiral arms or a well-defined disk. The overall appearance is consistent with that of an early-type galaxy undergoing some degree of passive evolution. There is a very subtle suggestion of some minor disturbance in the outer halo, though this could be noise. The galaxy does not appear to be undergoing a major merger.
