The galaxy appears as a slightly elongated, elliptical structure with a smooth, diffuse light distribution. The central region shows a concentration of light, brighter than the outer regions, possibly indicating a significant galactic nucleus. The color is generally yellowish-orange, suggesting a population of older stars. There is no noticeable spiral arm structure or dust lane features within the visible light spectrum. Minor asymmetrical features might indicate a past merger or interaction, but are subtle. The light distribution suggests a relatively evolved system with reduced star formation activity.
