The galaxy appears as a centrally concentrated, elliptical-like object. The core exhibits a strong yellow-white luminosity, suggesting a population of older, evolved stars. A faint, greenish halo surrounds the core, possibly indicating a small population of younger stars or ionized gas. The overall structure is smooth, with no apparent spiral arm structure or significant dust lanes visible in this image. The galaxy displays a high degree of circularity and doesn't appear to be undergoing any major merging activity, nor does it display evidence of tidal tails or other strong gravitational disturbances.
