The galaxy presents as a relatively smooth, elliptical-like structure with a concentrated central bulge. The light distribution suggests a generally spheroidal shape, though there are hints of slight asymmetry. The core region exhibits a bright, diffuse glow, with a less intensely illuminated halo extending outwards. There are no clear spiral arm structures visible; the overall appearance points toward a galaxy with older stellar populations and low recent star formation. The lack of distinct features suggests a relatively relaxed system, with no obvious signs of major disturbances or ongoing mergers. The color appears generally red, indicating that there is a lack of hot, young, blue stars, suggesting a more evolved system.
