The galaxy presents as a single, cohesive object with a smooth, elliptical morphology. A bright, concentrated core is evident, exhibiting a high degree of luminosity. The light gradually diffuses outwards from the core, transitioning into a less intense, yet still well-defined, outer region. The galaxy appears relatively undisturbed, lacking any obvious signs of spiral arms or significant tidal interactions. Color gradients are subtle, with a slight bluer hue in the outer regions suggestive of some ongoing star formation. The overall light distribution adheres closely to a Sersic profile, hinting at an old stellar population.
