The observed galaxy presents a largely elliptical morphology with a smooth, concentrated central bulge. The light distribution appears relatively uniform across the galaxy, with no prominent spiral arms or distinct features indicative of active star formation in a disk component. The primary color is a yellow-orange hue, suggesting a population of older stars and a relative lack of young, hot, blue stars. The shape is largely round and undisturbed, with no obvious signs of tidal interactions or ongoing mergers. There might be minor irregularities or subtle asymmetries in the outer regions of the galaxy that could be indicative of minor disturbances.
