The galaxy presents as a singular, centrally concentrated object with a relatively smooth overall morphology. It appears roughly elliptical in shape, showing high degree of circularity. There is a prominent, bright central region, indicative of a concentrated stellar population or potentially an active galactic nucleus. The color profile indicates the presence of a significant population of older stars. Star formation is estimated to be low. No clear spiral arms or disk-like features are discernible within the image, suggesting a lack of significant recent or ongoing merger activity. There are no obvious signs of major tidal disturbances or interacting companion galaxies.
