The galaxy presents a somewhat irregular morphology. A bright central region dominates, exhibiting a concentrated light profile. There are hints of a disk-like structure surrounding this central region, though its form is not well-defined. The overall color appears to be dominated by bluer wavelengths, particularly near the center, suggesting a population of younger stars. Fainter, redder patches can be seen on the periphery of the galaxy. There is evidence of possible disturbances in the galaxy's shape, potentially indicative of minor interactions or mergers. The edges appear somewhat ragged, with irregular extensions or features suggesting recent or ongoing activity. The galaxy does not appear to have a grand, symmetric spiral arm structure.
