The galaxy appears to be a luminous, relatively smooth elliptical galaxy, exhibiting a high degree of sphericity. It possesses a concentrated central bulge that emits strongly in redder wavelengths, indicating an older stellar population. There is no discernible spiral arm structure or significant dust lane obscuration visible. The galaxy shows no obvious signs of a recent or ongoing major merger event, though a faint asymmetry in the outer halo cannot be ruled out as a potential minor disturbance. The overall color suggests a relatively low ongoing star formation rate. The galaxy's estimated size indicates it is a massive system.
