The galaxy presents as a relatively smooth, elliptical structure with a high degree of central concentration. Its overall shape appears elongated. The color gradient suggests a population of older stars, particularly in the central bulge, which exhibits a yellowish-orange hue, indicative of evolved stellar populations. The outer regions show slightly bluer tones, hinting at the presence of younger stars or some level of ongoing, but low-level, star formation. There is no clear evidence of spiral arms or significant dust lanes. No major merger events are readily apparent, though the overall asymmetrical appearance implies a history of minor interactions, or disturbances. The galaxy appears mostly undisturbed.
