The galaxy exhibits a clear spiral structure. Two distinct spiral arms emanate from a central bulge. The arms are moderately wound. The bulge appears relatively small compared to the overall disk size. There appears to be a bar feature that spans almost the entire radius of the bulge. The disk is not viewed edge-on, presenting a more face-on orientation. The disk demonstrates some degree of clumpiness and inhomogeneity, suggesting ongoing or recent star formation activity. The spiral arms contain pockets of blue areas likely indicating regions of intense star formation. There are no major signs of tidal distortion or interaction with another galaxy, although there are some signs of minor disturbances in the disk.
