The galaxy presents as a centrally concentrated, elliptical-like structure. Its light profile appears smooth and diffuse, lacking distinct spiral arms or prominent dust lanes. The core exhibits a bright, yellowish hue, suggesting a population of older stars. The outer regions fade gradually into the background, indicating a decrease in stellar density with increasing radius. There may be a very slight disk, but this is difficult to discern from the image alone. There is no obvious signs of a major ongoing merger, though a minor disturbance cannot be ruled out. There is no obvious signs of star formation.
