The galaxy presents as an elliptical or lenticular type, exhibiting a smooth, centrally concentrated light profile. The core is bright and yellowish-white, suggesting an older stellar population. Moving outwards, the light gradually diminishes, transitioning to a reddish-orange hue. There is no apparent spiral arm structure or distinct dust lanes. The overall shape is moderately elliptical, without any signs of recent major merger events. Faint, diffuse light suggests a relatively smooth stellar halo extending outwards.
