The galaxy presents as an elliptical or lenticular type, exhibiting a largely smooth and centrally concentrated morphology. The light distribution appears centrally concentrated, with a significant fraction of the overall light emanating from a bright, somewhat diffuse core region. There are faint, asymmetric features, but are not a dominant part of the morphology. The color gradient suggests the presence of a more evolved stellar population in the central region. The galaxy appears to be relatively isolated with no obvious signs of recent or ongoing major merger activity.
