The galaxy presents as a spiral type, with a noticeable disk structure. Two well-defined spiral arms emanate from a central bulge. The arms display a somewhat flocculent morphology, exhibiting a medium to loose winding pattern. The central bulge appears moderately sized. The overall color gradient suggests a relatively high degree of ongoing star formation within the spiral arms, as indicated by their bluer hues, compared to the yellower central region which likely hosts an older stellar population. There is a slight indication of a bar-like structure crossing the central region. Certain regions of the disk show evidence of possible disturbances, potentially due to minor gravitational interactions. Overall, the galaxy presents itself as an actively star-forming system with a classic spiral morphology.