The galaxy presents as a somewhat elliptical, likely disk-shaped structure, viewed at a moderate inclination. The central region exhibits a bright, concentrated core, suggesting a significant concentration of older stars. The color gradient shifts from yellowish in the central bulge to a slightly bluer hue in the outer regions of the disk. There's a hint of spiral structure. The galaxy appears relatively undisturbed with no major signs of ongoing mergers or tidal features. Given the observed morphology, it is likely an evolved galaxy with moderate star formation.
