The galaxy presents as a roughly elliptical or spheroidal structure. The light profile appears relatively smooth and centrally concentrated. There is a distinct color gradient, with the core exhibiting a yellowish hue which may be indicative of an older stellar population. The outer regions transition to a slightly bluer tint implying a younger stellar population is located here. There is very little or no morphological evidence of a prominent disk or spiral arms, there are no obvious signs of recent or ongoing major merger activity. The smoothness indicates this galaxy likely is an elliptical galaxy.
