The galaxy appears to be a relatively smooth, elliptical-type galaxy, exhibiting a concentrated central bulge of older stars, indicated by its yellowish hue. The overall shape appears generally round to slightly elliptical. There's little evidence of prominent spiral arm structures or significant dust lanes. The galaxy seems to be relatively undisturbed with no major signs of tidal interactions or ongoing mergers. Some minor disturbances are present, possibly hinting at past interactions. The outer regions of the galaxy fade gradually, suggesting a smooth transition from the central bulge to the surrounding halo. The galaxy's colors suggest low to moderate levels of recent star formation.
