The galaxy presents as a relatively smooth, elliptical-like structure, with a high degree of central concentration. The light profile appears smooth and centrally peaked. There is a noticeable color gradient, with the core exhibiting a warmer, more yellowish hue compared to the outer regions, which show a slightly bluer tint. There is no clear evidence of spiral arms, a distinct disk structure, or significant dust lanes. No ongoing major merger activity is visible. The galaxy appears largely undisturbed.
