The galaxy appears to be a relatively bright, moderately sized elliptical. It is fairly smooth in appearance, lacking any distinct spiral arm structures or significant dust lanes. The color profile suggests an older stellar population, with a yellowish central bulge and a slightly bluer, though still overall aged, halo extending outwards. The light distribution indicates a centrally concentrated mass profile, which suggests a relaxed system that has undergone significant dynamical evolution. The galaxy appears isolated, showing no immediate signs of tidal interactions or ongoing mergers with neighboring galaxies, though minor disturbances cannot be ruled out at this resolution. The general morphology suggests that star formation is minimal. The roundness of the galaxy indicates that it is likely an E0 or E1 elliptical.
