The galaxy presents as a moderately luminous, bluish-white elliptical form. Its structure is dominated by a smooth, centrally concentrated light distribution. The central region exhibits a bright core, indicating a potentially active galactic nucleus or a high concentration of stars. The overall shape appears moderately elongated. The lack of distinct spiral arms or dust lanes suggest a more evolved system with ongoing or recently quenched star formation. Subtle indications of minor disturbances may point to past interactions, though the general morphology suggests a relatively settled system. The estimated size places it within the range of typical elliptical galaxies, and the color indicates a stellar population likely dominated by older, less massive stars.
