The galaxy presents as a somewhat amorphous, centrally concentrated object. It appears to possess a moderate degree of smoothness in its overall structure, although there are suggestions of faint, diffuse features extending from the central region. There is a suggestion of a disk component, but without clear spiral arms or a well-defined disk structure. The central bulge exhibits a yellowish hue, potentially indicating an older stellar population. The outer regions show a bluer tinge, hinting at the presence of younger stars and ongoing or recent star formation. The galaxy exhibits signs of gravitational interaction or a recent minor merger event, as evidenced by the slight asymmetry and subtle distortions in its overall shape. The luminosity is considerable, suggesting a relatively massive galaxy. The colors indicate it lies at an intermediate redshift. 
