The galaxy presents a largely smooth morphology, with a concentrated central region and a more diffuse, fainter halo extending outwards. Its overall shape appears elliptical, with a high degree of roundness. There is no obvious indication of spiral arm structures or significant dust lanes. The galaxy's color suggests an older stellar population, with a yellowish-red hue dominating the central bulge. The outer regions show a slightly bluer tint, potentially indicating the presence of younger stars, although this is subtle. There are no strong signs of ongoing major mergers or tidal disturbances, suggesting a relatively settled and evolved system. However, there might be very minor asymmetries that are too minor to note.
