The galaxy presents as a spiral type, displaying a clear disk structure. The spiral arms are well-defined, originating from a central bulge region. The arms exhibit a grand design, suggesting a well-ordered structure. Within these arms, there is evidence of active star formation, indicated by clumpy regions of bluer light. The central bulge appears yellowish in color and roundish, possibly indicating an older stellar population. The galaxy's disk is not perfectly edge-on, showing some inclination relative to our line of sight, allowing a glimpse of the spiral structure. The galaxy shows no signs of an ongoing major merger or significant tidal disturbances, though there is a hint of some subtle distortions. There are no visible bars across the galaxy's bulge. The central bulge is small compared to the entire structure of the galaxy, and overall the winding of the spiral arms appear to be moderate.
