The galaxy presents as a smooth, elliptical-like structure. It exhibits a high degree of central concentration, with a bright, moderately blue-shifted core. The light gradually diffuses outwards, lacking any distinct spiral arms or prominent features. The galaxy appears more elongated than circular, tending toward an in-between roundness. There are no obvious signs of on-going major mergers, although some minor disturbances can not be ruled out due to the slight asymmetry in the outer regions. The subdued color and smooth texture suggest a relatively quiescent galaxy, implying low levels of current star formation activity. The mass is substantial, characteristic of elliptical galaxies. The overall impression is that of a mature system, largely devoid of the dust lanes and HII regions often associated with active star formation.
