The galaxy presents as a single, concentrated body of light, exhibiting a smooth, elliptical morphology. A central, bright core emits a yellowish hue, suggesting a population of older stars or significant dust obscuration. The light intensity gradually diminishes outwards from the core, transitioning to a fainter, bluish halo. This halo is largely featureless, with no apparent spiral arms or prominent structures. The overall shape indicates a relaxed dynamical state, with minimal evidence of recent mergers or tidal disturbances, though subtle irregularities may be present upon closer inspection. The colour suggests ongoing but subdued star formation within the galaxy, contributing to its overall luminosity.
