The galaxy presents as an elliptical or lenticular type, exhibiting a smooth, centrally concentrated light profile. The core region appears bright and somewhat diffuse. The overall shape is close to round, with only a slight elongation. The color gradients suggest an older stellar population dominates, with a hint of bluer light indicative of some star formation. There is no obvious evidence of spiral arms, bars, or significant tidal disturbances. There are no clear signs of an active galactic nucleus based on its core and shape. The galaxy seems to be a relatively isolated system, with no obvious signs of recent or ongoing merger activity. The overall morphology indicates a galaxy that has likely undergone significant dynamical relaxation.
