The galaxy presents as a centrally concentrated object with a primarily smooth morphology. It exhibits a somewhat elliptical shape, deviating slightly from perfect circularity. A bright, yellowish core region is apparent, suggesting an older stellar population and likely the presence of a supermassive black hole. A fainter, more diffuse halo surrounds the core, displaying a bluer color. This indicates the presence of younger stars and ongoing or recent star formation, though at a relatively low rate. There is some evidence of minor disturbances in the outer regions of the galaxy, potentially from a past interaction or a minor merger event. The object does not appear to be undergoing a major merger at this time, nor does it show signs of strong tidal distortions. Overall, the galaxy appears to be a relatively evolved system.
