The galaxy presents as a relatively smooth, centrally concentrated structure. Its morphology appears largely elliptical, exhibiting a moderate degree of roundness in its overall form. The central region displays a bright, yellowish hue, indicative of an older stellar population and potentially a supermassive black hole actively accreting matter. A faint blue halo surrounds the central bulge, suggesting the presence of some younger stars or a low level of ongoing star formation activity. The galaxy does not show any obvious signs of major mergers or significant tidal disturbances. There is a minor irregularity on the side of the galaxy, suggesting that it could be either a minor disturbance, or simply another galaxy that happens to be in the background of the image. Based on its color and morphology, this galaxy is likely a relatively massive system.
