The galaxy presents as a spiral type, viewed approximately face-on. The spiral structure is fairly well-defined, with two prominent arms clearly visible. These arms exhibit a medium winding, not tightly wound but not particularly open either. These spiral arms appear to be populated with regions of active star formation, evidenced by their bluer color and irregular shapes.

The central bulge of the galaxy is relatively small compared to the overall disk. It appears yellowish-white in color, indicating a population of older stars. There is a hint of a possible bar structure, although it is not particularly prominent.

There appears to be signs of interactions going on with another galaxy. The shape of the spiral arms are warped, suggesting a possible tidal interaction with a smaller companion. There are disturbances in the general structure and a slightly asymmetric disk with clumpy features, which further indicates ongoing gravitational interactions or mergers. 
