The galaxy presents a generally smooth and rounded morphology. The light distribution appears concentrated towards the center, suggesting a prominent central bulge or core. The galaxy exhibits a moderate radial color gradient, transitioning from a yellowish-white core to a slightly bluer outer region. This may indicate differences in stellar populations and ages, with older stars concentrated centrally and younger stars forming in the outer regions. There's no clear evidence of spiral arm structures or significant dust lanes. Minor asymmetry is observed in the outer regions, possibly due to tidal interactions or minor disturbances, though no major merger is apparent. The galaxy's overall structure seems to be relatively undisturbed, indicating a quiescent evolutionary state.
