The galaxy presents as a relatively smooth, elliptical structure. Its core exhibits a bright, concentrated luminosity, suggesting a significant stellar density within the galactic center. The light profile appears to gradually diminish outwards from the core, lacking prominent spiral arms or distinct features usually associated with disk galaxies. The overall color is redder, indicative of an older stellar population and reduced recent star formation. There is little evidence of ongoing mergers or major disturbances in the morphology, although minor irregularities cannot be entirely ruled out at this resolution. The shape is generally round.
