The galaxy exhibits a spiral morphology, characterized by a central bulge and extending spiral arms. The spiral structure appears somewhat flocculent, with arm segments that are not continuous. There's evidence of active star formation within these arms, showing a bluer color. The bulge is a yellowish hue, suggesting an older stellar population. The galaxy is viewed at nearly face-on, and the image appears to indicate no signs of significant disturbances from any recent mergers, although subtle signs of possible past or minor interactions may exist in the outer regions of the disk. The galaxy displays no obvious strong central bar feature.
