This galaxy presents as a largely featureless, elliptical morphology, appearing quite smooth in structure. It exhibits a concentrated, bright core that gradually fades outwards into its extended halo. The color profile suggests an older stellar population, with a dominant yellowish-orange hue indicative of evolved stars. There is no obvious evidence of spiral arms or significant dust lanes. The overall round shape suggests a system that is close to relaxed, with little evidence of recent major merger activity or tidal disturbances. Based on its color and morphology, this galaxy appears to be an elliptical galaxy with a significant mass and low specific star formation rate.
