The galaxy presents as an elliptical or lenticular type. The object exhibits a smooth, centrally concentrated luminosity profile, with a gradual fall-off in brightness towards the outer regions, consistent with little dust or gas. The overall shape is moderately rounded. There is no obvious spiral structure, bar, or other significant features indicative of active star formation or significant dust lanes. There is no evidence of a major merger event, tidal tails, or other signs of recent interaction. A subtle color gradient appears present, with the core being redder in color than the outer halo.
