The galaxy presents as a largely featureless, elliptical morphology, with a high degree of smoothness. The overall shape appears somewhat rounded, exhibiting only a mild deviation toward a more elongated form. There is no apparent indication of significant tidal disturbances or ongoing mergers, though subtle asymmetries cannot be completely ruled out due to the image resolution.

Color gradients suggest a central concentration of older stellar populations exhibiting a redder hue, with the outer regions appearing slightly bluer, potentially indicative of a small amount of ongoing or recent star formation. The galaxy exhibits a relatively compact size. Based on the inferred redshift, this galaxy is significantly distant.
