The galaxy exhibits a spiral morphology, characterized by prominent spiral arms extending outwards from a central bulge. These arms display a clumpy structure, indicative of ongoing star formation regions. The bulge appears moderately sized. There is no clear indication of a strong bar structure. The overall color of the galaxy suggests a mix of stellar populations, with bluer regions associated with younger, hotter stars within the spiral arms, and a slightly redder hue towards the central bulge, potentially indicating an older stellar population. The galaxy presents an ordered structure with no signs of major mergers or significant disturbances, though some minor irregularity may be present. The disk appears inclined, but not edge-on.