The galaxy appears to be a smooth, elliptical structure with a high degree of central concentration. The light profile suggests a relatively old stellar population, as indicated by the smooth, featureless appearance and lack of discernible spiral arms or dust lanes. The object's shape is mostly round and is generally undisturbed by any major mergers with other systems. The estimated size of the galaxy is a few kiloparsecs in radius, which is not atypical for this type of galaxy. The core exhibits a high degree of luminosity, likely due to the high concentration of stars at the galactic center. A slight bluer tinge in the central regions compared to the outer halo could suggest a small amount of ongoing star formation, but the overall color indicates that this galaxy is populated mainly by older, redder stars. Overall, the data points to a well-formed elliptical galaxy in a relatively isolated environment.
