The galaxy presents a largely smooth morphology with some indication of internal structure. A dominant, centrally located component is characterized by a yellowish-orange hue, possibly indicating an older stellar population. There is a hint of an extended halo or diffuse emission surrounding this central region. Situated slightly offset is a smaller region exhibiting a bluish color, suggestive of ongoing star formation and a younger stellar population. Based on the proximity and morphology, it's plausible that this galaxy is undergoing a minor interaction or disturbance with the secondary region.
