The galaxy appears to be a spiral type, exhibiting a noticeable disk structure. The spiral arms are prominent and well-defined, with evidence of active star formation within them, indicated by a bluer hue in these regions. The central bulge is moderately sized relative to the disk, exhibiting a yellowish-white color, suggesting an older stellar population. There is a suggestion of a bar-like structure in the central region, though its strength is difficult to determine given the image resolution. The galaxy does not appear to be undergoing any major merging events, but there is some indication of minor disturbances in the disk, possibly due to interactions with smaller companion galaxies or internal processes. The disk is not observed edge-on.
