The galaxy presents as a relatively compact spiral structure, exhibiting a defined disk component. The spiral arms appear loosely wound, extending outwards from the central region, but are not fully well defined, possibly indicating flocculent characteristics. Multiple arms can be differentiated. A central bulge is present, and it appears relatively modest in size but has a large radial size. There is no indication of a strong central bar feature, however there appears to be a weak presence of one. A hint of some kind of disturbance in the structure. The disk is not seen perfectly edge-on, but close.
