The galaxy presents as a single, centrally concentrated object with a generally smooth morphology. Its light profile appears largely elliptical with a high degree of roundness. The core region exhibits a bright yellowish-white color, suggesting a population of older stars. There is a slight color gradient outward from the core, transitioning to a redder hue in the outer regions, which could indicate ongoing, but relatively low star formation. There is no apparent disk structure, spiral arms or signs of a recent major merger event. The smooth appearance and color profile indicate that this galaxy is most likely an elliptical galaxy in which star formation has largely ended.
