The galaxy presents as a relatively smooth, centrally concentrated elliptical morphology. The light profile appears largely featureless, with a high degree of rotational symmetry. Color gradients are subtle, transitioning from a yellowish core to slightly redder hues in the outer regions. There is no distinct bulge or disk visible at this resolution. The galaxy appears generally isolated, showing no signs of tidal interactions or major disturbances with neighboring galaxies. The spheroidal shape and color suggest a population of older stars dominates the stellar content.
