The galaxy presents a distinct spiral structure. Two spiral arms can be clearly discerned, exhibiting a moderate winding pattern as they extend from the central bulge. The bulge appears to be of moderate size, contributing significantly to the overall luminosity of the galaxy. The galaxy exhibits a central bar-like structure.

There is no clear evidence of a recent major merger. The galaxy has a notable star formation rate, as indicated by its color, but not enough to change it's type. The galaxy is observed at a redshift implying a considerable distance. The estimated size of the galaxy suggests it is a substantial object.
