The galaxy presents a generally smooth and elliptical morphology. It displays a concentrated central bulge exhibiting a yellowish-orange hue, suggesting an older stellar population and a low rate of ongoing star formation. The outer regions of the galaxy appear fainter and redder, extending into a somewhat diffuse halo. There is no discernible evidence of spiral arms or a distinct disk structure. The overall appearance suggests a relaxed system without any signs of significant ongoing merger activity or major tidal disturbances. Its round shape indicates it is most likely an elliptical galaxy.
