The galaxy presents a predominantly smooth morphology. The central region exhibits a high degree of concentration, appearing nearly spheroidal. The overall shape is somewhere between round and elongated, with a color profile that trends towards bluer hues in the outer regions. It shows no obvious signs of a disk structure, spiral arms, or a central bar. There is no clear indication of recent or ongoing major merger activity, although minor asymmetries or disturbances cannot be entirely ruled out. The galaxy's apparent size is relatively small, suggesting a moderate physical size. The light is dominated by older stellar populations.
