The galaxy presents as an elliptical, exhibiting a smooth and relatively featureless morphology. It displays a high degree of central concentration, with the luminosity decreasing smoothly from the core outwards. The overall shape is moderately elongated, with a ratio of the minor to major axis approximating 0.8. Color gradients are subtle, with the central region appearing slightly more yellowish than the outer regions, suggesting a population of older stars in the core. There is no evidence of spiral arms or prominent dust lanes. The galaxy appears relatively isolated, with no obvious signs of interaction with neighboring galaxies.
