This galaxy presents as an elliptical, non-spiral type. The core region exhibits a bright, yellowish-white hue, indicating a concentration of older stellar populations. Moving outward from the core, there's a gradual transition to a fainter, more diffuse halo. Subtle color variations within the outer regions suggest possible ongoing, albeit low-level, star formation. The overall morphology indicates a relatively undisturbed system, lacking any prominent tidal features or signs of recent merger activity. The galaxy appears moderately massive. The light distribution suggests it is neither perfectly spherical nor significantly elongated.
