The galaxy presents a slightly elongated, elliptical appearance. The central bulge exhibits a bright, yellowish hue, suggestive of an older stellar population. The outer regions display a bluer coloration, indicating the presence of younger stars and ongoing star formation, albeit at a low rate. There is evidence of faint, disturbed features. It appears that there may have been a small gravitational disturbance in the past, which explains the overall shape. Overall, it presents properties between an elliptical and a spiral galaxy.