The galaxy exhibits a generally smooth morphology with a dominant central bulge. There is little evidence of spiral arm structure or distinct features, suggesting it may be an elliptical galaxy or a lenticular galaxy seen face-on. The central region is significantly brighter and appears reddish-orange, potentially indicating an older stellar population and/or dust obscuration. The outer regions of the galaxy are less luminous and display a hint of bluer colors, which could indicate the presence of younger, hotter stars in lower densities compared to the core. The overall shape is approximately circular, with minimal elongation or distortion visible. There's no clear indication of ongoing merger activity or significant tidal disturbances. The relatively compact size and brightness profile suggest a massive galaxy.
