The galaxy presents as a single, relatively smooth object with a high degree of central concentration. The primary body of the galaxy exhibits a near-spherical morphology, though it is not perfectly round, showing a slight elongation or cigar shape to one side. The central region is significantly brighter than the outer regions, suggesting a dense core population, such as an active galactic nucleus or a high concentration of stars. Diffuse features are visible, with hints of disrupted structures which could possibly be a merger. There are color variations across the galaxy, with the central region appearing bluer, and the outer regions appearing redder. The blue color could be associated with ongoing star formation, and the redder color could be due to older stellar populations.
