The galaxy presents as a singular, relatively smooth object with a dominant central bulge. There is minimal visual evidence of spiral arm structures or dust lanes. The overall shape appears mostly round, though not perfectly circular. It exhibits a concentrated luminosity profile, with the majority of light emanating from the core. Color gradients suggest a possible variation in stellar populations, with the central region displaying a bluer hue, potentially indicating younger stars or active star formation. The outskirts appear redder, possibly due to older stellar populations. Tidal disturbances, merging features, or nearby companion galaxies are not immediately apparent in the image. The overall appearance suggests a relatively evolved galaxy.
