The galaxy presents a largely smooth, elliptical morphology. The light profile appears concentrated toward the center, with a radially decreasing intensity outward. The galaxy exhibits a yellowish-white hue, suggesting a dominant population of older stars. There is little indication of spiral arm structures or significant dust lanes. The galaxy appears largely undisturbed, showing no signs of major mergers or tidal interactions. There are a few faint, very subtle color variations that could indicate a small amount of ongoing, low-level star formation, but overall the galaxy appears quiescent.
