The galaxy presents an elliptical morphology, appearing primarily smooth in structure with a slight degree of elongation. Its color profile indicates a redder, more evolved stellar population, suggesting a lack of significant recent star formation. The object appears to be largely undisturbed, without evidence of ongoing mergers or major tidal interactions. It is moderately bright and relatively compact, indicative of a high mass concentration. The galaxy exhibits an overall undisturbed form with a dominant spheroid.
