The galaxy presents as a spiral morphology with a distinct disk. The spiral arms appear well-defined, with a tightly wound structure in some regions and more open in others. The arms exhibit a predominantly blue coloration, suggestive of ongoing star formation. There may be two main spiral arms with hints of other arms. The bulge is moderately sized and is a yellow-orange color, indicating an older stellar population. The galaxy's disk is not perfectly face-on, but is inclined at a small angle with respect to our line of sight. The overall color of the galaxy ranges from blue in the arms to yellow/orange in the central bulge region. There is possible interaction or distortion in the disk, which suggests a minor merger. There is evidence for star formation.
