The galaxy presents as a relatively smooth, elliptical morphology with a high degree of roundness. The color profile suggests a prominence of older stellar populations, with the galaxy appearing more reddish in the core and outer regions. There is minimal evidence of significant star formation activity, as indicated by the lack of strong blue hues associated with young, hot stars. No distinct spiral arms or a well-defined disk structure are apparent, supporting the classification as an elliptical galaxy. There is no visual indication of any recent major merger events or tidal disturbances. The galaxy exhibits a centrally concentrated light profile with a gradual decline in intensity towards the edges.
