The galaxy appears as a centrally concentrated, elliptical or lenticular-like structure. It exhibits a smooth, diffuse morphology with a dominant bulge component. The galaxy displays a color gradient, with a yellowish-red hue in the central region and a gradual transition to a bluer periphery. There are no discernible spiral arms or prominent dust lanes. There is no apparent ongoing major merger activity or strong tidal distortions, but potentially some evidence for a minor disturbance. The galaxy appears relatively isolated within the field of view.
