The galaxy presents as an elliptical morphology, potentially a disk galaxy viewed at a relatively high inclination angle. It exhibits a smooth appearance with a concentrated central bulge. The color profile suggests an older stellar population. The lack of distinct spiral arms and the relatively uniform color distribution further imply that star formation is somewhat suppressed within the galaxy. A subtle asymmetry in the overall shape hints at possible minor gravitational interactions or past merger events. A small green hue at the very center implies that there is an emission line present, perhaps a region with more active star formation.