The galaxy exhibits a prominent disk structure with evidence of spiral arms. These arms appear somewhat tightly wound, indicating a possible grand design spiral morphology. A notable bulge is present at the galaxy's center. The overall color suggests a mix of stellar populations, with a central yellowish hue potentially indicating older stars in the bulge, while bluer tinges may indicate ongoing star formation within the disk and spiral arms. A possible central bar feature is noted running through the middle of the galaxy. There are no signs of any kind of major merging occurring but minor disturbances can not be ruled out.
