The galaxy presents as a moderately elliptical system, elongated along its major axis. The central bulge region exhibits a relatively smooth, concentrated appearance with a yellow-orange hue, suggesting an older stellar population. The outer regions display a fainter, bluer color, hinting at some ongoing star formation, although likely at a low rate. There is little discernible disk structure or spiral arm morphology. The overall appearance indicates a galaxy that is largely devoid of significant morphological disturbances or signs of recent major merger events. Based on the observed morphology, the galaxy appears to be transitioning towards a more quiescent state.
