The galaxy presents as a relatively smooth, elliptical structure with a concentrated central bulge. The light distribution appears largely uniform, lacking prominent spiral arms or distinct features indicative of active star formation. The galaxy exhibits a slightly elongated shape, deviating marginally from a perfect circle. There is a subtle color gradient, with the core appearing more yellow/white and the outer regions taking on a slightly reddish hue. This suggests an older stellar population concentrated in the center with potentially younger stars in the outer regions. There are no obvious signs of tidal disturbances or ongoing mergers.
