The galaxy presents as a singular, largely featureless object. Its morphology is dominated by a smooth, elliptical appearance. There is a concentration of light towards the center, indicating a central bulge. Color gradients suggest a relatively homogenous stellar population with older stars dominating. The object exhibits a notable degree of sphericity and minimal signs of tidal disturbances or ongoing mergers. There is a slight asymmetry in its light distribution, although that might be due to image imperfections. Any spiral arm structure or dust lanes are not apparent, suggesting it is either absent or are very subtle.