The galaxy presents as a primarily smooth, elliptical form. Its core region exhibits a high degree of luminosity, suggesting a concentrated stellar population and possibly an active galactic nucleus. The overall color profile indicates a significant presence of older stellar populations, appearing reddish-yellow in the observed bands. Subtle asymmetries or disturbances are discernible in the outer regions, hinting at potential past interactions or minor disturbances affecting the galaxy's morphology. A faint, possible tidal tail or extended feature can be observed, though definitive classification requires further investigation. The galaxy's general structure lacks prominent spiral arms or well-defined features typically associated with actively star-forming galaxies.
