The galaxy presents as a moderately luminous, ellipsoidal structure, exhibiting a centrally concentrated light profile. The core displays a yellowish-white hue, indicating a population of older stars. The outer regions appear reddish, suggesting the presence of dust lanes that obscure some of the bluer light from younger stars. A slight asymmetry is noticeable, possibly indicative of a minor interaction or disturbance. Star formation appears to be relatively suppressed. The overall morphology suggests a system transitioning towards a more passive, quiescent state.
