This galaxy exhibits a relatively smooth morphology, with a high concentration of light towards the center. The galaxy's shape appears to be somewhere between round and elliptical, showing a slight elongation. There is little evidence of spiral arm structures or distinct features suggesting an ongoing major merger event. Some minor disturbances might be present. The light is dominantly in the blue-green spectrum, possibly indicating recent or current star formation. It exhibits a low to moderate star formation rate, along with a stellar mass range between 10^9 and 10^10 solar masses. The galaxy is relatively compact. Overall, based on the image and measured data, this appears to be a galaxy in the process of transitioning toward a more passive and spheroidal morphology.
