The galaxy presents as a spiral type, with a prominent disk structure. The spiral arms appear somewhat tightly wound near the central bulge, becoming less defined and looser further out. The central bulge exhibits a moderate size relative to the disk and demonstrates a distinct reddish hue, possibly indicating an older stellar population. The overall color of the disk is primarily bluish, suggestive of ongoing star formation. No strong bar feature is discernible. There is a slight indication of a possible minor disturbance or interaction occurring, evident by a subtle asymmetry or distortion in the outer disk.
