The galaxy exhibits an overall smooth morphology, with a high degree of circularity. The light distribution is concentrated towards the center, fading gradually outwards. There is a slight hint of a disk structure. There are no obvious signs of spiral arms or a prominent bar. The galaxy has a yellowish-white hue, suggesting a relatively older stellar population. There is no strong evidence of active star formation regions. The light is distributed relatively uniformly with a high amount of smoothness, and no major disturbances apparent from mergers or tidal interactions are visible. 
