The galaxy presents as a spiral type, exhibiting prominent, well-defined spiral arms. These arms appear open and extend outwards from a central bulge region. The bulge component appears relatively small, though noticeable. There is evidence of active star formation within the arms, as indicated by the patchy distribution of bluer, younger stellar populations along their lengths. The overall color of the galaxy appears somewhat blue-shifted suggesting a moderate level of on-going star formation throughout the disk. The disk of the galaxy is viewed at an angle that is neither face-on nor edge-on, providing a clear view of the spiral structure. There is a possible weak bar structure bisecting the bulge, however the resolution is not high enough to confirm the presence of one. There may be some minor irregularities or disturbances in the outer regions of the disk, possibly resulting from minor interactions with other galaxies.
