The galaxy exhibits an elliptical morphology with a noticeable bulge. It presents a smooth texture, lacking significant visible dust lanes or spiral arm structures. The color profile suggests an older stellar population, with a central concentration of yellowish light, potentially indicating a population of evolved stars. The isophotes appear consistently elliptical, showing no strong signs of recent mergers or tidal disturbances beyond some possible warping. The overall light distribution follows a Sersic profile, suggesting it is an elliptical galaxy. It shows that this galaxy is redder in color, meaning that there is not a lot of star formation occurring in the galaxy.
