The galaxy presents a distinct spiral structure. Two prominent spiral arms emerge from the central region, exhibiting a moderately wound morphology. The central bulge appears substantial and is primarily yellow, suggesting an older stellar population. The spiral arms display a bluer hue, indicative of ongoing star formation.  A weak bar structure is suggested by the slight elongation of the central region. No signs of major mergers or significant tidal disturbances are readily apparent. The galaxy is not viewed edge-on.
