The galaxy appears to be an elliptical type, exhibiting a largely smooth and spheroidal morphology. The central region displays a concentrated luminosity, suggesting a significant stellar density. The color gradient transitions from a yellowish-white core to a more diffuse, slightly bluer outer halo, potentially indicating a difference in stellar populations or dust content between these regions. There are some subtle irregularities, like the slight lopsidedness on the bottom, indicating possible ongoing or recent interaction or merging events. Overall, the galaxy's appearance is consistent with a massive system with moderate star formation.
