The galaxy appears to be an elliptical galaxy, exhibiting a generally smooth, concentrated light profile. The core region displays a bright, yellowish-white hue, which suggests a population of older stars. There is no clear indication of spiral arms or significant dust lanes. The overall shape is mostly round, with a slight deviation toward an in-between elliptical form. Faint extensions of light emanate from the core, fading gradually into the background, indicating a diffuse halo structure. There are no obvious signs of major mergers or significant tidal disturbances, though minor asymmetries cannot be entirely ruled out at this resolution. Overall, this galaxy seems to be a relatively quiescent system with a dominant population of older stars and minimal ongoing star formation.
