The galaxy presents as a spiral with well-defined, tightly wound arms. There is a small, but pronounced central bulge that appears bright. There is a defined disk that is at an angle from our point of view. The galaxy appears slightly elongated. The distribution of light suggests a mix of stellar populations with some concentrations of star formation within the spiral arms. Based on the color gradients, the galaxy shows signs of ongoing star formation. There is no clear evidence of a bar structure. Additionally, there is no evidence of a major merger event. The galaxy appears to be relatively isolated.
