The galaxy presents an elliptical morphology, with a smooth, concentrated central region. The luminosity profile appears to be centrally peaked. The galaxy displays a yellow-orange color in the core that fades to a more green-red hue as the radius increases, suggesting a significant population of evolved stars with minimal ongoing star formation. There may be a faint disk-like structure present with little to no spiral arms. There is no indication of major tidal disturbances or ongoing mergers in the image, though there seems to be some minor disturbance. The isophotes appear generally regular, with a slight elongation, suggesting it is not perfectly spherical. Overall, the galaxy appears to be a massive system with a high degree of symmetry and likely to be an older system.
