The galaxy presents a distinct disk-like morphology, observed at a slight angle relative to edge-on. A central bulge is evident, estimated to be moderate in size relative to the overall structure. Spiral arms are a prominent feature, with a structure most likely containing two arms, displaying a medium winding. There is a strong suggestion of a bar-like structure running through the central region of the galaxy, though a confirmation of its presence requires higher resolution imaging.

The light distribution indicates ongoing star formation, the color gradients suggest a higher rate of star formation in the arms compared to the bulge.

The overall appearance suggests the galaxy is in a relatively undisturbed state, showing no significant signs of major mergers or tidal interactions. Minor disturbances may be present.
