The galaxy presents as a slightly elliptical, relatively smooth structure. There is a concentration of light toward the central region of the galaxy, which appears to be a yellowish or gold hue, possibly indicative of an older stellar population. Fainter, diffuse light extends outward from this core, displaying a bluish-green tint. This suggests the presence of younger stars or regions of active star formation. The overall morphology suggests an intermediate stage of galaxy evolution, possibly transitioning from a spiral-like structure to a more elliptical form. There is a hint of minor irregularity in the outer regions. No strong indication of recent major mergers is apparent.