The galaxy presents a primarily smooth, elliptical morphology, appearing concentrated and relatively featureless in the optical bands. It exhibits a yellowish hue throughout the main body, suggesting an older stellar population with diminished recent star formation activity. The galaxy shows a slight elongation, deviating marginally from a perfect circular shape. Faint hints of disturbance are present within the galaxy; there appear to be some minor irregular structures in the outer edges of the galaxy. Although it is faint, the galaxy displays a bluer tint in the surrounding regions. These characteristics could be caused by recent or ongoing galaxy merger.
