This galaxy presents as a concentrated, elliptical morphology. The light distribution is centrally concentrated with a smooth radial falloff. There is a color gradient visible with a yellower hue towards the core that fades to redder color at the outskirts. There is no evidence of spiral arm structure. No distinct tidal features or strong signs of ongoing mergers are apparent. Faint disturbances may exist, but the data does not allow for a higher classification than minor disturbance. The galaxy appears relatively undisturbed. Based on the smoothness and color profile, the galaxy is likely to be a relatively massive, evolved system with little ongoing star formation. The general shape of the galaxy is more round than elongated. 
