The galaxy presents as a centrally concentrated object with a smooth, largely featureless morphology. Its overall shape approximates a rounded form, exhibiting a high degree of radial symmetry. There is no apparent evidence of spiral arms or a prominent disk structure. The light distribution appears relatively uniform, fading gradually from the bright central region outwards, without significant irregularities or clumpy features. There is no apparent evidence of strong tidal interactions or ongoing major merger events, although the possibility of subtle disturbances cannot be completely ruled out at this resolution. The color profile suggests a population dominated by older stars.
