The galaxy presents as a centrally concentrated, largely featureless system. Its overall shape is somewhere between round and elongated. There is a smooth gradient of light intensity from the core outwards, with no distinct spiral arms or bar structures readily apparent. The color profile suggests a dominant population of older stars, with a yellowish-orange hue throughout the galaxy's body. There are no apparent signs of major ongoing mergers, although subtle irregularities may indicate minor past interactions or internal disturbances. Overall, the galaxy appears to be an evolved system, potentially nearing a more quiescent stage of stellar formation.
