The galaxy presents a largely smooth, elliptical morphology. The color profile suggests a dominant population of older stars, with a central concentration exhibiting a yellowish-orange hue. Fainter, bluish regions are present in the outer edges, potentially indicative of some recent, yet minor, star formation activity. No distinct spiral arm structures are apparent. There is a slight irregularity in the outer halo's shape, possibly suggesting a minor past interaction or disturbance, but no major merging events are readily visible. Overall, the galaxy appears to be a relatively evolved, massive system experiencing a low level of ongoing star formation.
