The galaxy presents as a diffuse, extended object. The overall morphology is generally smooth, but subtle features are apparent upon closer inspection. There is a hint of a possible disk-like structure, though the galaxy appears somewhat irregular rather than a well-defined spiral or elliptical. There are also disturbances in its morphology, indicating either minor or major disturbances, perhaps from a past merger. The object exhibits color variation across its body, with the redder light seemingly more concentrated toward the center, suggesting a possible older stellar population in the core. Fainter blueish regions are also present.
