The observed galaxy presents a primarily smooth morphology, exhibiting a notable lack of discernible spiral arms or distinct substructures within its overall form. The central region displays a concentrated luminosity, suggesting the presence of a substantial galactic nucleus. The galaxy's shape is elliptical, leaning towards a more rounded appearance, but not perfectly circular, possessing a slight elongation. The color profile indicates a higher intensity in the redder bands with the green band also present. Faint structural disturbances are present, hinting at a possible interaction or merger event in the galaxy's past. The central region seems to be intact with no major visual signs of disruption. Overall, the galaxy appears relatively quiescent, consistent with an evolved stellar population.
