The galaxy exhibits a spiral morphology, characterized by prominent spiral arms emanating from a central region. The spiral arms are well-defined and extend outwards. The winding of these arms appears moderate. The central bulge displays a moderate size relative to the disk and exhibits a yellowish color, possibly indicating an older stellar population. The galaxy disk presents a bluer hue indicative of younger stars within the arms. There is a hint of bar structure present, with potentially a weak or strong bar component. The galaxy is not observed edge-on. There appears to be no major signs of merging or tidal disruption, but minor disturbances might be present. Overall, the galaxy appears to be a typical spiral galaxy.
