The galaxy presents a largely smooth, elliptical morphology. Its light profile appears concentrated towards the center, with a gradual decline in intensity outwards. The color is predominantly a yellow-white hue, suggesting an older stellar population, particularly in the core. There is little evidence of distinct spiral arms or dust lanes. Subtle color variations might indicate minor variations in stellar populations or metallicity across the galaxy, but these are not highly pronounced. Overall, the galaxy appears as a relatively undisturbed system without significant ongoing star formation.
