The galaxy appears to be a relatively smooth, elliptical galaxy, likely a spheroid with minimal discernible substructure. Its light profile indicates a centrally concentrated morphology. The color suggests a population of older stars, resulting in a yellowish-orange hue, with a hint of green, indicating a possible small amount of ongoing star formation. The galaxy exhibits a high degree of circularity in its overall shape. There is no apparent indication of any major mergers or tidal disturbances affecting the galaxy.
