The galaxy appears as a centrally concentrated object with a smooth, elliptical morphology. It is generally circular in shape. The galaxy exhibits a dominant bluish-white hue in its central region, gradually fading outwards. There is minimal evidence of spiral arms or distinct disk structures in this image. The light distribution suggests a relatively uniform stellar population. Signs of merging or major disturbances are not readily apparent. There may be some minor asymmetry. The observed color is consistent with a moderate redshift.
