The galaxy presents as a generally smooth, elliptical structure with a bright, concentrated central bulge. The core exhibits a yellowish-white hue, suggesting a population of older stars. Moving outward from the core, the color transitions towards a redder, slightly less luminous halo. There is a faint suggestion of a disk component, displaying very subtle features or disturbances, possibly indicative of minor interactions or internal processes. The galaxy is not perfectly spherical, displaying an intermediate flattening of the central bulge. There is no strong evidence of ongoing major merging activity or significant tidal tails. The color gradients suggest a relatively quiescent star formation history, more representative of an evolved system.
