The galaxy appears to be an elliptical galaxy, characterized by a smooth, spheroidal morphology with a high degree of central concentration. The core is bright and yellowish, indicating an older stellar population. There is a gradual decrease in luminosity from the center outwards, with no distinct spiral arms or a prominent disk structure visible. The color suggests relatively low ongoing star formation, dominated by older, redder stars. There are no obvious signs of tidal disturbances or major mergers, suggesting it has been relatively undisturbed recently. Overall, the galaxy presents a fairly evolved and relaxed system.
