The galaxy presents as a spiral type, viewed at a slight angle from face-on. Two prominent spiral arms are clearly visible, loosely wound around a central bulge. The central bulge appears relatively moderate in size. There is faint evidence of a bar-like structure running through the central region. Disk extends beyond the bulge and spiral arms, the outer parts of which are mottled in appearance. There are minor disturbances in the disk of the galaxy, though no major merging activity is apparent.
