The galaxy appears to be an elliptical galaxy exhibiting a relatively smooth morphology. It is characterized by a central bulge, with a diffuse, faint halo extending outwards. There are faint indications of possible mergers or tidal disturbances in the outer reaches of the halo. The galaxy presents with an intermediate roundness, not perfectly spherical but also lacking a highly elongated shape. The galaxy exhibits intermediate star formation activity. The core of the galaxy exhibits different spectral properties, including a lower redshift than the outer reaches, suggesting a rotating core.