The galaxy presents as a relatively smooth, elliptical-like structure with a prominent central bulge. Its color profile suggests an older stellar population, exhibiting a yellowish-orange hue in the core region that transitions to a bluer periphery. There is some indication of a faint, diffuse disk surrounding the central bulge, but distinct spiral arms are not apparent. The galaxy appears largely undisturbed, with no major signs of ongoing mergers or tidal distortions. Minor asymmetries are present.
