The galaxy presents a somewhat elliptical morphology, appearing moderately smooth in structure. A concentrated central bulge is discernible, exhibiting a yellowish-white hue, indicating an older stellar population. Surrounding the bulge is a diffuse disk component, which is less defined and appears bluer in color. The blue tint suggests ongoing star formation within this region. The overall roundness suggests that it is not a spiral galaxy. There is a slight asymmetry and minor disturbances present in the outer disk.
