The galaxy presents as a spiral galaxy, observed at an angle that suggests it's not quite edge-on, nor is it perfectly face-on. There's evidence of prominent spiral arm structures, although the resolution of the image limits detailed observation of individual star forming regions within them. The color distribution indicates a central bulge that appears yellower, potentially indicating an older stellar population. The disk appears bluer in comparison, possibly suggesting ongoing star formation. A relatively small bulge may be observed within the galaxy, but its difficult to definitively classify any bar-like structures within the image. The overall morphology of the galaxy seems relatively undisturbed.