The galaxy presents a largely smooth, elliptical morphology. It exhibits a concentrated, rounded shape, lacking prominent spiral arms or a distinct disk structure. The light distribution appears relatively uniform across its body, suggesting an older stellar population with reduced ongoing star formation. There is a subtle colour gradient visible, the core appearing slightly more yellow/red than the outer regions, which could indicate a difference in stellar population or dust content between these areas. Any disturbances or signs of interaction with other galaxies appear to be minimal; the galaxy seems generally isolated and relaxed in its morphology.