The galaxy appears to be a relatively smooth, elliptical galaxy. It exhibits a centrally concentrated light profile with a bright, yellowish core that gradually fades towards the outer edges. The overall shape is elongated, suggesting a classification of type E3-E5 on the Hubble sequence. There is little evidence of spiral arms or significant dust lanes. Color gradients are subtle, but a slight bluer hue can be discerned towards the outer regions, potentially indicating the presence of a younger stellar population compared to the core. There does not appear to be any signs of tidal disruption or ongoing merger activity.
