The galaxy presents a flattened, disk-like structure, characteristic of a spiral galaxy. Evidence of spiral arms is present, although somewhat tightly wound. The central bulge is moderately prominent and exhibits a yellowish hue, potentially indicative of an older stellar population. The arms themselves show a bluer coloration, which suggests ongoing star formation. There is no visual evidence of a major merger, though some minor disturbances in the disk structure might be present. The galaxy is relatively large, spanning an estimated diameter on the order of several kiloparsecs. No strong bar feature is discernible. There may be some asymmetry.
