The galaxy presents as an elliptical morphology, exhibiting a smooth, concentrated central bulge that dominates the overall structure. The light distribution appears relatively uniform, lacking prominent spiral arms or distinct features indicative of recent or ongoing mergers. The color profile suggests a primarily older stellar population, with a yellowish hue characteristic of evolved stars. There is little evidence of dust lanes or significant star formation regions. The galaxy is nearly round, with a slight ellipticity. Based on its apparent color and smoothness, it is likely a massive galaxy with a low star formation rate.