The galaxy presents a generally smooth morphology, appearing largely featureless and diffuse. Its overall shape is approximately round, with a high degree of circular symmetry. There is a noticeable concentration of light toward the central region, suggesting a well-defined galactic nucleus or bulge. The galaxy does not exhibit any obvious signs of major disturbances or ongoing mergers. Its color suggests an older stellar population, or a lack of significant recent star formation. The size appears to be on the larger end.
