The galaxy presents as a centrally concentrated system, likely elliptical in morphology. The core is a bright, compact region, appearing yellowish in color. The surrounding halo exhibits a more diffuse, bluish glow, indicating the presence of a distinct stellar population, perhaps with ongoing, or recent, star formation. The object presents an overall smooth appearance, suggesting that it may have a simple, undisturbed structure. There is faint suggestion of a very weak and diffuse, distorted arm feature at the outer edge of the object to the right. The galaxy's shape is somewhere between round and elongated. There is no evidence of a significant major merger currently in progress, although there is evidence of minor disturbance within the galaxy. The light from this distant galaxy has shifted to redder wavelengths due to its motion away from us.
