The galaxy presents a generally smooth and elliptical morphology. A bright, concentrated central bulge dominates the structure, suggesting a high stellar density in this region. The galaxy exhibits a noticeable color gradient, transitioning from a bluer hue in the outer regions to a yellower color towards the center. This could be indicative of varying stellar populations and ages across the galaxy, with potentially older, redder stars concentrated in the bulge. There's a very slight hint of a disk structure, but it's not prominent. No spiral arms are discernible. The galaxy appears relatively undisturbed, showing no major signs of ongoing mergers or significant tidal interactions. There is very minor clumpy structure within the disk, but the galaxy is mostly homogeneous.
