The galaxy presents a roughly elliptical morphology with a bright, concentrated core. The light distribution appears smooth, lacking any distinct spiral arm features or prominent dust lanes. The color profile suggests a generally older stellar population, with a slight reddening towards the core and a bluer hue in the outer regions, which is common with elliptical galaxies. There is no apparent disturbance or tidal features suggesting a recent major merger event. The overall structure indicates a galaxy that is relatively undisturbed and quiescent in its evolutionary state.
