The galaxy presents as a relatively smooth, elliptical or lenticular structure. It exhibits a generally rounded morphology with a high degree of central concentration. There is no strong evidence of spiral arms or a prominent disk component. Faint hints of a diffuse halo may be present, but its extent and structure are difficult to discern. The galaxy appears to be in a relatively quiescent state, with no obvious signs of ongoing major mergers or significant tidal disturbances. A very compact, bright core is visible, possibly indicating the presence of an active galactic nucleus, or simply a dense concentration of stars. Overall, the galaxy appears to be a mature system, likely comprised predominantly of older stellar populations. The color indices suggest a moderate redshift, consistent with a considerable distance from the observer.
