The galaxy presents as a centrally concentrated, elliptical-like structure with a smooth, diffuse appearance. The core region exhibits high luminosity, gradually decreasing outwards. There are no apparent spiral arms or prominent dust lanes, indicating a lack of significant recent star formation in the outer regions. The overall color is subtly red, with some faint blue tinges in the outer regions. The galaxy appears relatively isolated, showing no signs of major ongoing mergers or tidal disturbances. The shape is generally round, with only a slight elongation. It is likely a massive galaxy given its absolute magnitude and inferred stellar mass, with a relatively low star formation rate.
