The galaxy presents as a slightly elliptical structure with a bright, concentrated central bulge. The core exhibits a yellowish-orange hue, indicative of an older stellar population. Surrounding the central bulge is a fainter, more diffuse disk. The disk shows subtle hints of spiral arm structure, though these are not well-defined. The outer regions of the disk appear smoother with a relatively low level of star formation. There are no obvious signs of major mergers or significant tidal disturbances. Overall, the morphology suggests a galaxy with characteristics somewhere between a spiral and a lenticular galaxy.
