The galaxy presents a generally smooth and rounded morphology. The central region exhibits a bright, concentrated core, suggestive of a substantial stellar population or an active galactic nucleus. This core is surrounded by a more diffuse halo of light that extends outwards. There is a hint of a disk-like structure, but it is not prominent. There is very little disturbance, hinting at the lack of a major merger, though there might be a minor disturbance. Colors within the galaxy vary, the central area being slightly redder/yellower, with the outer regions exhibiting bluer tones.
