The galaxy presents as a singular, relatively smooth object, with a concentrated central bulge that is luminous. The shape appears predominantly elliptical, exhibiting a high degree of circularity. The outer regions of the galaxy gradually fade into the background sky, indicating a lack of defined spiral arms or other complex structures. There is no apparent sign of ongoing merger activity, such as tidal tails or distorted morphology. The color profile suggests an older stellar population, with a lack of blue light indicating low recent star formation.
