The galaxy presents a largely smooth, elliptical morphology. There is minimal indication of spiral arm structures or dust lanes within the observed image. It appears predominantly spheroidal, with a high degree of central concentration. The color profile indicates a potential mix of stellar populations, with a yellowish-orange core possibly indicative of older stars. A slightly bluer, greener halo surrounds the core, suggesting the presence of some younger stars. There is no clear evidence of ongoing major mergers or significant tidal disturbances. The galaxy appears relatively isolated and undisturbed.
