The galaxy presents as a spiral type, exhibiting prominent, well-defined spiral arms that appear somewhat tightly wound. The disk structure is clearly visible, showing a slight inclination. There is a distinct central bulge that is moderately sized. The galaxy's color profile indicates active star formation regions within the spiral arms, evidenced by their bluer tint, while the bulge appears yellower, suggesting an older stellar population. A bar structure appears to be present. There are no obvious signs of a major ongoing merger. The morphology indicates some disk features.
