The galaxy presents as a relatively smooth, elliptical structure with a high degree of central concentration. The core exhibits a bright, yellowish-white hue, indicative of an older stellar population. A faint, diffuse halo surrounds the central region, extending outwards in a slightly elongated form. The light distribution suggests a minimal presence of dust lanes or prominent spiral arms. There are no visible signs of recent major merger activity or significant tidal disturbances. The overall morphology is consistent with an early-type galaxy, potentially an elliptical or lenticular galaxy in a relatively quiescent state.
