The galaxy presents as a relatively smooth, elliptical morphology. The luminosity profile indicates a concentration of light towards the galactic center, with a gradual decrease in surface brightness as radial distance increases. Color gradients are subtle, with a slightly yellower core transitioning to a redder halo. There is no prominent disk structure visible, nor any clear indications of spiral arms or active star formation regions. The galaxy appears largely undisturbed, without any signs of ongoing major mergers or tidal interactions.
