The galaxy presents as a largely smooth, elliptical-like structure. The central region exhibits a high degree of luminosity, appearing almost uniformly bright with a slight color gradient towards the center. The color distribution is dominated by blue and white hues in the core, suggesting a population of younger stars. The outer regions of the galaxy are less defined, showing a gradual decrease in luminosity and a transition to slightly redder colors. There is a faint indication of some minor disturbances in the shape of the galaxy, possibly due to past interaction. However, the overall morphology leans towards a relatively undisturbed system. 
