The galaxy appears as a centrally concentrated object with a relatively smooth overall morphology. The core region exhibits a bright, almost point-like structure, surrounded by a more diffuse, less intense halo. A slight elongation is visible in the image. The central region displays a light blue color. There is evidence of some internal structure within the galaxy, hinting at the possibility of a weak or poorly defined disk. Given the light blue core, we can expect there to be a relatively low rate of star formation in this galaxy. The overall structure suggests the galaxy is relatively undisturbed, showing no major signs of tidal interactions or recent mergers, although a minor disturbance cannot be ruled out.
