The galaxy presents as a single, concentrated light source, appearing largely smooth and elliptical in shape. It exhibits a noticeable color gradient, shifting from a predominantly orange-red hue at its core to a greenish-yellow tinge at its periphery, suggesting potential differences in stellar populations or dust content across the galactic body. There is no visual evidence of spiral arms or a distinct disk structure; rather, its morphology is more consistent with a spheroid. I see no strong tidal features, distortions, or other signatures of an ongoing or recent major merger event, and the galaxy generally appears undisturbed.
