The galaxy presents a generally smooth morphology, appearing nearly elliptical in shape. It exhibits a dominant central bulge that transitions gradually into a surrounding halo. Color gradients suggest a higher concentration of older stellar populations in the central regions, which appear redder in comparison to the outer regions. The outer regions have a slightly bluer hue and contain faint, unresolved features. Overall, there is little evidence of spiral arms or active star formation present. There do not appear to be any signs of recent or ongoing galaxy merger activity.
