The galaxy presents as a centrally concentrated, elliptical-like structure. The core exhibits a distinct yellowish-orange hue, suggesting a population of older stars. There is a surrounding halo that graduates to greenish-yellow. The object appears generally smooth with no clear signs of distinct spiral arms or a bar structure. There are no signs of substantial tidal disturbances or major mergers, though subtle asymmetrical features may suggest a minor interaction in its past or ongoing. The overall morphology indicates a relatively evolved system.
