The galaxy presents as a spiral type, exhibiting a disk-like structure with evident spiral arms. These arms are prominent but lack tight winding, appearing more open and extended. The galactic bulge is relatively small, contributing less to the overall light profile. The image suggests a galaxy where star formation may be active within the spiral arms, as inferred by subtle color variations. Evidence indicates this is likely not a face-on view of the galaxy, but an angled view, as some of the disk features have been obscured. The galaxy displays a subtle asymmetry, with its spiral arm structure appearing slightly more prominent on one side than the other. The galaxy is of medium apparent brightness. There is a noticeable absence of a strong bar-like feature traversing the galactic center. There are some hints of minor irregularities in the galactic structure.
