The galaxy appears as an elliptical or lenticular type, exhibiting a generally smooth morphology. It presents with a concentrated central bulge, and a diffuse halo extending outwards. There is a slight deviation from a perfect circular shape, potentially indicating some minor gravitational interaction or internal dynamics. The galaxy exhibits a yellowish-white hue, suggesting a stellar population dominated by older, less massive stars. There is little to no discernible evidence of active star formation regions, spiral arm structures, or significant dust lanes within the galaxy. There are also no signs of an ongoing major merger with another galaxy. The galaxy exhibits a color gradient, appearing somewhat bluer in its outer regions and redder in its central regions. 
