The galaxy presents as a centrally concentrated system with a bright, nearly spherical core. There appears to be a faint, diffuse halo extending outwards from the core, exhibiting a subtle elongation or flattening along one axis. Color gradients are subtle, with the central region appearing bluer than the outer regions. Based on its smoothness and high central concentration, this galaxy likely has a high mass and a low specific star formation rate. There is slight evidence of disturbance, perhaps a minor merger in the galaxy's recent history.
