The galaxy presents a generally smooth and elliptical morphology, though there are some minor irregularities. The light distribution suggests a relatively high degree of central concentration. The galaxy exhibits a subtle color gradient, trending from slightly redder hues at the core to slightly bluer hues in the outer regions. There is evidence of a possible interaction or merger event, indicated by a slight disruption in the shape of the galaxy. Overall, the galaxy appears to be a fairly evolved system, consistent with it being an elliptical galaxy.
