The galaxy presents as a spiral type, viewed at an angle that is neither face-on nor edge-on. The presence of spiral arms is strongly suggested, tracing a pattern across the galactic disk. These arms are moderately wound. A prominent central bulge exists, exhibiting a concentrated luminosity, with the bulk of the bulge being of a moderate size. There are possible indications of a weak bar structure within the central region. The disk shows clumpy regions of star formation and regions of dust extinction. There may be an interaction of some sort happening in the lower portion of the galaxy, indicated by a region of blue. There are no indications that it is undergoing a major merger or disturbance. Overall, the galaxy exhibits characteristics of ongoing, substantial star formation.
