The galaxy presents as a luminous, elliptical-shaped object, exhibiting a smooth, centrally concentrated light distribution. It appears relatively featureless, with a notable absence of distinct spiral arms or prominent dust lanes. The core region displays a high surface brightness, indicating a dense concentration of stars. The outer regions gradually fade into the background, lacking sharp boundaries. The galaxy's color appears to be dominated by redder wavelengths, suggesting an older stellar population. The overall morphology indicates a classification toward the elliptical end of the Hubble sequence.
