The galaxy presents a largely smooth and rounded morphology. It exhibits a prominent, concentrated central bulge with a yellow hue, suggesting an older stellar population likely composed of Population II stars. The outer regions of the galaxy display a fainter, more diffuse halo. There's very little evidence of spiral arm structure or distinct features indicative of ongoing, rapid star formation. The overall structure appears relatively undisturbed, lacking significant signs of recent mergers or tidal interactions. The faint blue tinge in the outer halo could be due to a small population of young stars. This galaxy appears to be an elliptical galaxy and is likely to be a quiescent, massive galaxy with a low star formation rate.