The galaxy presents a smooth, elliptical morphology, with a high degree of central concentration. The light distribution appears largely spheroidal, lacking any readily discernible spiral arm structure or a prominent disk. The galaxy exhibits a gradual decrease in surface brightness from the core outwards. The central region is characterized by a bright, diffuse glow. Color gradients are subtle but suggest a redder core compared to the outer regions, possibly indicative of an older stellar population towards the center. There is no obvious evidence of recent major mergers or tidal disturbances. The overall appearance is consistent with a relatively evolved galaxy with a suppressed star formation rate.
