The galaxy presents as a relatively smooth object, with a dominant central bulge exhibiting a high degree of radial symmetry. There's a subtle transition from the brighter core to the outer regions. While a disk component is not entirely absent, it does not exhibit a high degree of structure or distinct spiral arms. A slight extension can be seen in the morphology of the object. The light distribution indicates that it is in an intermediate stage of morphology, between a spiral and elliptical galaxy. The color suggests ongoing star formation at a low rate. The object does not show any obvious signs of a recent major merger event, though some minor disturbances cannot be entirely ruled out.
