The galaxy presents as a spiral type with a moderate bulge, though the central bulge is not overly pronounced and blends smoothly into the galactic disk. High likelihood of containing spiral arms. The disk appears relatively face-on from our viewing angle. Evidence of ongoing star formation is present, with a bluer color on the arms. There is no evidence of a strong bar structure. The overall structure appears relatively undisturbed, lacking strong indications of a major merging event or significant tidal distortions. There may be slight irregularities in the disk, but it could be a minor disturbance. The galaxy is not edge on. 
