The galaxy presents a primarily smooth morphology, although there are subtle features that suggest the presence of a disk-like structure. The central region exhibits a concentrated bulge with a yellowish hue, indicating an older stellar population. The outer regions show a bluer color, possibly suggestive of more recent star formation. Faint, disturbed structures are present, which may suggest some sort of minor merger or tidal interaction. These appear as slight irregularities in the overall elliptical shape.
