The galaxy presents as a spiral galaxy, exhibiting a distinct disk structure. A bulge is visible, though it does not appear dominant in size relative to the overall galactic structure. The spiral arms are well-defined and loosely wound, tracing outwards from the central bulge. Two dominant arms are clearly observed. There are indications of ongoing star formation within the arms, evidenced by bluer hues within those regions. There may be some distortion of the disk, possibly due to gravitational interactions. There is no clear sign of an on-going merger, though minor tidal disturbance cannot be ruled out. A bar structure is present within the bulge, but is not particularly pronounced.
