The galaxy presents a largely smooth, elliptical morphology. The central region exhibits a bright, concentrated core with a yellow hue, suggesting a population of older stars. There is a gradual decrease in luminosity moving outward from the center, with the outer regions exhibiting a faint reddish tint. There's no clear evidence of spiral arms or significant dust lanes, but some minor irregularities in the overall shape suggest the possibility of a past interaction or minor disturbance.
