The galaxy presents as a somewhat centrally concentrated, lenticular system. The core region appears bright and yellow/white, indicating an older stellar population. The galaxy lacks distinct spiral arm structures or significant dust lanes. There is a smooth transition from the core to the outer regions, with a subtle blue shift in color, suggesting the presence of some younger stars within the extended disk. Faint irregularities are present in the outer regions of the galaxy, but no strong tidal features or signs of major recent merger activity are detected. The morphology suggests a relatively evolved system, possibly undergoing passive evolution or possessing low levels of ongoing star formation.
