This galaxy presents a complex morphology, primarily exhibiting characteristics of a spiral galaxy viewed at a moderate inclination. The central bulge appears relatively prominent, with a moderate size compared to the overall galactic disk. The disk shows evidence of prominent spiral arm structures. These spiral arms have a defined presence, generally exhibiting a tightly wound structure across the galactic disk. There is strong evidence of an internal bar structure crossing the central bulge. The bar appears to be quite extended, and is thin. The color distribution across the galaxy suggests a degree of ongoing star formation within the arms, indicated by bluer hues, while the bulge exhibits yellower colors, potentially signifying an older stellar population. There are possible signs of minor disturbances to the overall shape and structure of the galaxy, however there does not appear to be any major disturbance in the overall structure of the object, and does not appear to be merging with any other galaxies.
