The galaxy presents a generally smooth, elliptical morphology. It appears largely featureless, lacking prominent spiral arms or a distinct bar structure. The galaxy exhibits a centrally concentrated luminosity profile, with the brightness gradually decreasing towards the outer regions. The core region displays a yellowish-orange hue, potentially indicative of an older stellar population. There is some evidence of a faint, diffuse halo surrounding the main body of the galaxy. The overall shape appears mostly round, showing minimal deviation from a circular form. There is little evidence of ongoing or recent major merger activity.
