The galaxy presents as an elliptical system with a smooth, centrally concentrated light distribution. There is a clear color gradient, with a redder core transitioning to a bluer outer halo. The overall shape appears mostly round with a slight elongation along a single axis. There is no evidence of distinct spiral arms, bars, or other prominent features typically associated with disk galaxies. There appears to be no signs of tidal disturbances or ongoing merger activity. The central region is notably bright. The galaxy appears to be an evolved system, consistent with a high fraction of older stellar populations, which may have relatively low levels of ongoing star formation.
