The galaxy appears as a relatively smooth, centrally concentrated object. Its morphology is generally elliptical, exhibiting a high degree of sphericity with a slight deviation towards an intermediate shape.  There is a clear absence of strong spiral arm structures or significant disk-like features.  The galaxy's color gradient suggests an aging stellar population. The central region displays a brighter, more concentrated luminosity, surrounded by a fainter, more diffuse halo. Evidence of any major or minor mergers is minimal, with only the possibility of very slight disturbances. The galaxy seems to be at considerable cosmological distance, indicated by its small angular size and redshift. This suggests a mature system with relatively low star formation, dominated by older stars and potentially a supermassive black hole at the center.
