The object appears to be a spiral galaxy, seen at a slight angle relative to edge-on. The spiral arms are visible, displaying a relatively open structure. They appear somewhat flocculent in nature. There is evidence of ongoing star formation within these arms, indicated by their blueish hue. A central bulge is present, and the disk fades into the background. The galaxy shows a degree of asymmetry. There is no evidence of a strong bar feature. Based on the apparent light distribution, it appears to have a moderate to small-sized bulge. There are no obvious signs of a major ongoing merger, although there are hints of minor tidal disturbances or interactions.