The galaxy exhibits a centrally concentrated morphology, appearing largely smooth with a dominant, bright core. Its overall shape is moderately elliptical, tending toward roundness. The color gradient suggests an older stellar population, particularly concentrated within the central bulge, giving it a yellowish-red hue. There is a subtle, fainter extension or possible tidal feature located off-center, which could indicate minor gravitational interaction. The presence of this feature may suggest an ongoing or recent interaction. No prominent spiral arms or dust lanes are clearly discernible. Overall, the galaxy appears as a relatively undisturbed system, possibly in late-stage evolution.
