The galaxy presents a generally smooth and elliptical morphology. Its core exhibits a bright, concentrated luminosity, diminishing outwards. The color profile suggests a population dominated by older stars. Evidence of spiral arms or significant disk structure is absent. The galaxy appears relatively undisturbed with no prominent signs of ongoing mergers or major tidal interactions with other galaxies. There are no notable dust lanes visible within the galaxy's structure. It shows a redshift indicating it is at a considerable cosmological distance.
