The galaxy presents as a spiral type, exhibiting a clear disk structure. The spiral arms appear well-defined, winding moderately around the galactic center. There is a noticeable bulge, classifiable as moderate in size, occupying a significant portion of the central region. The presence of a bar structure is indicated, appearing somewhat strong. Star formation is apparent, as suggested by the presence of blue and yellow hues within the disk, potentially indicating active star forming regions. The galaxy does not exhibit any major signs of ongoing or recent major mergers, although the possibility of minor disturbances cannot be ruled out.
