The galaxy presents as an elliptical morphology, exhibiting a smooth, concentrated light profile. The core region is characterized by a bright, yellowish-white hue, indicating a concentration of older stellar populations. Moving outwards from the core, the luminosity gradually diminishes, transitioning to a fainter, reddish-orange color. There is no discernible spiral arm structure or distinct dust lanes. The overall structure suggests a relatively quiescent galaxy with minimal ongoing star formation. The smoothness and rounded shape point to an evolved system that has undergone significant dynamical relaxation. No evidence of major mergers or tidal disturbances is apparent in this image, though very minor disturbances cannot be ruled out.
