The galaxy presents as a centrally concentrated object, exhibiting a largely smooth morphology with a high degree of roundness. There is a dominant, bright central region that diminishes in intensity with increasing radius. Evidence of a disk-like structure is minimal, and the galaxy appears to be primarily spheroidal. No significant tidal features or prominent dust lanes are discernible. There appears to be minimal star formation, as implied by the subtle color gradients observed. There are no other obvious signs of recent or ongoing mergers.
