The galaxy presents as a centrally concentrated object with a smooth, elliptical morphology. The color gradient transitions from a bright, yellowish core to a fainter, slightly redder halo. There is no apparent structure, such as spiral arms or dust lanes visible in this image. The smooth light distribution suggests a relatively old stellar population dominating the galaxy's light output. Given its color and shape, it is likely an elliptical galaxy with ongoing, moderate star formation. There may be minor disturbances in its structure, but overall it seems largely undisturbed, indicating a low likelihood of recent major mergers.
