The galaxy presents as a single, dominant spheroid structure with a smooth, elliptical morphology. The light profile appears centrally concentrated with a bright, unresolved core. There are no apparent spiral arms or a distinct disk component visible. The galaxy exhibits a color gradient, transitioning from a yellowish-white core to redder outer regions. This suggests an older stellar population is dominant within the core. The overall structure indicates a lack of significant ongoing star formation and suggests a high probability that this is an elliptical galaxy. There is no obvious evidence of tidal disturbances or merger activity.
