The galaxy presents as a centrally concentrated, elliptical-like structure. The core exhibits a bright, yellowish-orange hue, suggesting an older stellar population likely dominated by red giant stars. The light is relatively smooth, without prominent dust lanes or spiral arm structures visible. The galaxy's overall morphology appears quite regular, with minimal signs of recent merger activity or major tidal disturbances. There is potentially a small satellite galaxy or background object close to the center of the primary object. Overall, the galaxy appears to be in a relatively quiescent state, without substantial ongoing star formation activity in the nuclear region. 
