The galaxy presents a largely smooth, elliptical morphology. It exhibits a concentrated central bulge, diminishing in luminosity towards the outer edges with no resolved spiral arms. The galaxy appears to be quite round in shape. There is a subtle colour gradient from the center to the edges, with the central regions appearing slightly more yellow, potentially indicating an older stellar population. There is no obvious indication of a major ongoing merger, although slight distortions are possible. Overall, the galaxy appears to be a relatively undisturbed, evolved system.
