The galaxy presents as a spiral type, characterized by a flattened disk-like structure. Within this structure, two prominent spiral arms emanate from a central region, displaying a medium to loose winding pattern. These arms are distinct and traceable, appearing somewhat flocculent in nature.  A moderate degree of star formation is apparent within the arms, evidenced by the presence of several localized regions of bluer light, suggestive of younger stellar populations. The central bulge appears relatively small and not particularly bright, giving the disk a more dominant visual presence. There may be a bar structure present, but this is hard to confirm visually. Overall, there do not appear to be any major signs of recent mergers or significant tidal disturbances. The galaxy is inclined relative to our line of sight, appearing somewhat oval in shape.
