The galaxy presents a largely featureless morphology, appearing smooth and elliptical in shape. Its color profile indicates a prominent red core, transitioning outwards to a less concentrated, greenish halo. There's little evidence of spiral arms or distinct disk-like structures. The galaxy's overall form is relatively uniform, lacking significant tidal tails, distortions, or other indications of ongoing major merger activity. Subtle irregularities on the periphery suggest possible minor disturbances, or interactions but these are not very apparent. The luminosity appears to be concentrated toward the center, consistent with a higher density of stars and older stellar populations.