The galaxy presents as a relatively smooth, elliptical morphology. The central bulge exhibits a high degree of luminosity, with the intensity decreasing gradually towards the outer regions. The overall shape appears elongated, rather than perfectly spherical. There are no prominent spiral arms or distinct features indicative of active star formation visible in this imaging. There are subtle variations in color across the galaxy, with the central bulge exhibiting a slightly yellower hue compared to the outer regions, which tend towards redder tones. There are no visible signs of any significant merger events.