The galaxy presents as a somewhat elongated, disk-like structure with a distinct central bulge. The central region appears to be dominated by older stellar populations, exhibiting a yellowish-orange hue. Surrounding the core, a flattened disk is observed, showing hints of spiral structure with a greenish tint. This suggests the presence of younger, bluer stars and potentially ongoing star formation within these outer regions, with the older regions appearing more red. The morphology indicates that the galaxy is relatively undisturbed, with no obvious signs of major mergers or significant tidal interactions.
