The galaxy presents as an elliptical morphology, appearing largely smooth with a high degree of central concentration. It exhibits a roughly round shape, with only slight deviations from perfect circularity. There is no immediately discernible spiral arm structure, bar, or other prominent features typically associated with disk galaxies. Color gradients are present, with a yellowish hue concentrated toward the center, subtly shifting towards a redder coloration in the outer regions. There is no evidence of ongoing major or minor merger activity, or significant tidal disturbances in its immediate vicinity. The galaxy appears to be a relatively isolated system in this field of view.
