The galaxy presents as a concentrated, elliptical structure with a smooth, featureless morphology. Its color profile suggests a dominant population of older stars, likely exhibiting minimal ongoing star formation. The central region shows a higher concentration of light, indicative of a possible galactic nucleus. There is no clear indication of spiral arms or a distinct disk component. The galaxy appears relatively isolated, with no visually apparent signs of tidal interactions or mergers. Its overall rounded shape implies a dynamically relaxed system. The apparent red-shift suggests the galaxy is located at a considerable distance.
