The galaxy presents a primarily smooth morphology with a concentrated central region. There is a slight elongation indicating it is not perfectly circular. Color gradients are present, with a central region appearing more luminous and exhibiting a greenish-yellow hue, possibly indicative of older stellar populations. Fainter and bluer extensions are present and appear to be some sign of disturbances. These disturbances could be due to a minor merger. The overall structure appears somewhat diffuse, and the galaxy does not exhibit well-defined spiral arms or a prominent disk.
