The galaxy presents a largely smooth, elliptical morphology. There is a distinct central bulge, which appears bright and concentrated. The galaxy lacks prominent spiral arms or a well-defined disk structure. The overall color appears slightly yellow to orange, suggesting a relatively older stellar population. There are no obvious signs of ongoing major mergers or significant tidal disturbances, though subtle irregularities in the outer regions might indicate minor interactions. The galaxy exhibits a high degree of radial symmetry, with the light distribution decreasing smoothly from the core to the outer edges. Based on the image, it appears to be a relatively massive galaxy with a low star formation rate.
