The galaxy appears to be a luminous, elliptical galaxy. The central bulge exhibits a concentrated, bright yellowish hue. The galaxy exhibits a generally smooth morphology with a slight falloff in brightness from its center to its periphery. There is no obvious spiral structure or dust lanes visible, which suggests a relatively old stellar population and a lack of significant ongoing star formation. The galaxy's round shape indicates minimal rotational support and a relatively isotropic velocity dispersion of its constituent stars. A possible faint halo surrounds the main body of the galaxy, which could be either extended stellar populations. There seems to be no sign of major mergers or tidal disturbances present in this image.
