The galaxy presents an elliptical morphology, appearing largely smooth with minimal discernible substructure. It is concentrated, with a higher density core that fades away into diffuse edges. Its color is generally reddish-yellow, suggestive of an older stellar population. There is a slight blue hue at the outer edges, which may indicate the presence of younger stars. Overall, the galaxy does not present any strong tidal features, signs of significant ongoing mergers, or active galactic nuclei.
