The galaxy appears as a centrally concentrated, roughly elliptical object. It exhibits a smooth, largely featureless morphology with a high degree of central light concentration. There is no discernible spiral arm structure or obvious dust lane features present within the optical range depicted. The color gradient suggests an older stellar population dominates, exhibiting a yellowish hue, which may indicate suppressed star formation. The overall rounded shape points towards a likely classification as an elliptical galaxy. There is very subtle evidence that this galaxy is undergoing some interaction with other galaxies, as it exhibits a slight disturbance in its otherwise smooth morphology.
