The galaxy exhibits a clear spiral structure, with two prominent arms originating from the central bulge. The arms appear somewhat tightly wound and can be traced for a significant portion of the galaxy's radius. The color gradient indicates the presence of a notable central bulge, which appears yellowish, suggesting an older stellar population. The disk shows a bluer hue indicating active star formation. There appears to be a subtle asymmetry, possibly indicative of a minor gravitational interaction. 
