The galaxy presents as a slightly elongated structure with a bright, concentrated central bulge that dominates the overall light output. The bulge appears relatively smooth and featureless. Surrounding the bulge is a fainter, more diffuse disk, oriented approximately vertically in the image. The disk component exhibits a gradual decline in brightness moving away from the central bulge. The galaxy appears to be an early-type spiral or a lenticular galaxy. The general morphology appears relatively undisturbed, with no obvious signs of recent major merger events or tidal interactions. The galaxy appears to be in a relatively isolated environment.
