The galaxy presents as a luminous, elliptical form with a high degree of central concentration. A bright, yellowish core region dominates the galaxy's morphology, suggesting an older stellar population with minimal ongoing star formation. The isophotes appear relatively smooth, lacking any distinct spiral arm structures or prominent dust lanes. There is a subtle flattening of the galaxy along its major axis and an axial ratio of approximately 0.3. The light appears to decrease smoothly and gradually from the center toward the outer regions, without sharp edges or breaks. Overall, the galaxy appears as an elliptical galaxy.
