The galaxy presents as a centrally concentrated object, likely an elliptical. It exhibits a smooth, almost featureless morphology with a high degree of central symmetry, appearing nearly circular in shape. The light distribution suggests minimal dust obscuration. The galaxy's color profile indicates a relatively red color in the central region, transitioning to a slightly bluer hue in the outer regions. This color gradient implies a generally older stellar population in the core and the potential presence of younger stars in the outer regions, though overall star formation appears to be minimal. There is no evidence of significant tidal disturbances or ongoing major mergers. A slight asymmetry hints at a possible minor interaction.
