The galaxy presents as a centrally concentrated object with a smooth, relatively featureless appearance. It exhibits a roughly elliptical morphology, appearing more circular than elongated. The light distribution appears to be generally uniform, with a gradual decrease in intensity from the core outwards. The central region displays a yellowish hue, suggestive of an older stellar population. The outer regions show a bluer color, possibly indicating the presence of younger stars or ongoing star formation, though this is not strongly pronounced. There is no obvious presence of spiral arms or a prominent disk structure. There is a lack of any major disturbances in the overall shape, indicating that no major mergers or interactions are occurring with other galaxies, though some minor disturbance cannot be ruled out. 
