The galaxy appears to be a relatively smooth, elliptical or lenticular system. Its morphology is characterized by a centrally concentrated, bright core with a diffuse halo extending outwards. The light distribution suggests a predominantly old stellar population. There is no obvious presence of spiral arms or significant dust lanes. The object appears slightly elongated, deviating from a perfectly circular shape. Minor disturbances are potentially present within the structure. No signs of a major merger or interaction with a companion galaxy are visible within this field of view.