The galaxy appears as a centrally concentrated luminous object. It exhibits an elliptical morphology with a relatively smooth light distribution, showing no distinct spiral arm features or obvious substructures. The color gradient suggests a redder core, possibly indicating an older stellar population dominating the central region. The outer regions seem to exhibit bluer tones compared to the core. The galaxy is moderately bright. There are no signs of any strong tidal disturbances or ongoing major mergers. The overall appearance is consistent with that of an early-type galaxy, potentially an elliptical or lenticular galaxy. There seems to be a degree of asymmetry in its outer halo region.
