The galaxy presents as a single, relatively smooth concentration of light. It exhibits a generally elliptical morphology, appearing mostly round with minimal elongation. The primary color is a warm yellow-orange hue, suggesting a population of older stars. There is no discernible spiral structure or prominent dust lane visible. The light distribution is fairly uniform, with a gradual decrease in intensity from the central region outwards, lacking any strong point sources or distinct features indicative of recent or intense star formation. It shows no visible signs of major interactions or mergers.
