The galaxy presents as a centrally concentrated object, exhibiting a smooth, largely featureless morphology. Its overall shape appears moderately elliptical. A bright, condensed core is evident, suggesting the potential presence of a supermassive black hole actively accreting material, or a high concentration of stars in the galactic nucleus. The color profile indicates a bias toward redder wavelengths, which may be indicative of an older stellar population and a low rate of star formation throughout the galaxy. There are no apparent spiral arms or significant dust lanes visible in this image. No signs of a major ongoing merger are visible.
