The galaxy presents a largely smooth, elliptical morphology. The light profile appears centrally concentrated, with a gradual decline in brightness outwards from the core. There is no discernible spiral arm structure or prominent disk. The overall shape is relatively round, with a minor deviation from perfect circularity. There is no apparent evidence of ongoing major merging events or tidal disturbances. Color gradients within the galaxy suggest a population of older stars, with a slight bluer color trend in the outer regions.
