The galaxy presents as a centrally concentrated, elliptical morphology. The light distribution appears smooth with a high degree of central concentration, indicative of an older stellar population. No spiral arms or prominent dust lanes are visible. The isophotes exhibit a generally rounded shape, trending slightly towards a flattened ellipsoid, with the major axis having no clear orientation. The color is predominantly redder, suggesting a dearth of recent star formation. There is no evidence of any ongoing or recent merger activity. The galaxy is relatively compact in appearance, with the majority of its light concentrated within a small region.
