The galaxy appears to be a relatively smooth, elliptical system. The central region exhibits a bright, concentrated core, suggesting a high stellar density. The color gradient transitions from a reddish-orange hue in the core to a bluer tint in the outer regions, which may indicate a change in stellar populations from older stars at the center to younger, hotter stars further out. There is no clear evidence of spiral arm structure or a prominent disk component. The overall shape is generally round with some hints of slight elongation. There may be some minor disturbances present in its shape, but no major mergers or signs of ongoing interactions are observed.
