The galaxy presents as a relatively face-on spiral system, though with some inclination. There's evidence of a central bulge that emits strongly in shorter wavelengths. It's surrounded by a relatively flat and thin disk which itself demonstrates spiral structure. The disk appears to be rich in young stars and star-forming regions as indicated by the relatively blue emissions in some areas of the disk and the redder emissions towards the outer areas, suggesting areas of dust extinction, older stellar populations, or active star formation. The galaxy does not appear to be undergoing any major merger events, with no obvious tidal tails or strong morphological disturbances. There are slight asymmetries in the outer disk region, suggesting a possible minor interaction in the past. The galaxy appears to be fairly compact.
