The galaxy appears to be a relatively smooth elliptical galaxy with a concentrated central bulge. The light profile exhibits a high degree of central concentration, diminishing gradually towards the outer regions. There are no visible spiral arms or other distinct features indicative of recent or ongoing major mergers. The galaxy's shape is nearly circular, suggesting a low degree of rotational support. The color is generally yellow-white, possibly indicating an older stellar population with a low rate of star formation. Given the smoothness, roundness, and color, this galaxy is likely a relatively massive system composed primarily of older stars, with a supermassive black hole residing at its center.
