The galaxy presents an elliptical morphology, appearing largely smooth in texture. The overall shape approximates an ellipse, showing a moderate elongation. Its color profile shows a central concentration that appears yellowish-white, suggesting an older stellar population within the core. There are no distinct spiral arms or prominent dust lanes visible. Marginal evidence points towards a quiescent star formation rate and a large mass. No signs of strong gravitational disturbances or ongoing major merging events are visible.
