The galaxy presents as a generally smooth and elliptical object, with no immediately discernible spiral arm structure. There is a bright, concentrated central bulge that exhibits a yellow-orange hue, suggesting an older stellar population dominating the core. Moving outward from the center, the galaxy's luminosity decreases gradually. The outer regions appear more diffuse and less defined. It is likely that the galaxy is a massive system, with a moderate amount of ongoing star formation. There's no obvious visual evidence of a major merger event, though some minor distortions might be present in the outer halo. The galaxy is located at a considerable distance, exhibiting a moderate redshift. The shape is somewhere between round and elongated.
