The galaxy presents as an elliptical structure with a smooth morphology. The galaxy exhibits a notable color gradient, with a bright, slightly elongated core. The core appears almost white, suggesting a population of hot, young stars or potentially AGN activity. Surrounding the core is a greenish halo. The light is more diffuse than the core and extends outwards. The light begins to fade, shifting towards a pinkish-purple hue. The galaxy has a cigar shape. The overall structure indicates that the system is relatively undisturbed, lacking any obvious signs of recent major mergers or tidal interactions. The distribution of light suggests a relatively stable stellar population.
