The galaxy presents a roughly elliptical morphology, although there appears to be some structural disturbance. Its central region is characterized by a bright, concentrated bulge. The bulge exhibits a yellowish hue, suggesting an older stellar population with fewer young, massive stars. Fainter, diffuse light extends outward from the core, forming a halo or disk-like structure. Some evidence suggests the possibility of an ongoing merger event, with asymmetrical distortions visible in the outer regions of the galaxy.
