The galaxy presents as a singular, dominant structure, appearing generally smooth in texture. The morphology indicates a high degree of central concentration. The overall color is suggestive of an evolved stellar population, trending towards redder wavelengths. There is little to no apparent substructure, such as spiral arms or prominent dust lanes, within the galaxy's profile. The light distribution suggests a centrally concentrated spheroid, with a gradual decline in luminosity outwards. The object exhibits a round shape, showing a largely undisturbed and relaxed morphology. There's no obvious sign of on-going merger activity or significant tidal disturbances in the immediate vicinity. The relatively compact appearance suggests a high-mass system with a low star formation rate.
