The galaxy exhibits a distinct spiral structure, characterized by two prominent, well-defined arms that appear to wind moderately tightly around a central bulge. The bulge component seems of moderate size, contributing significantly to the overall luminosity of the galaxy's central region. The arms display a relatively smooth texture, suggesting active star formation is limited, which is corroborated by the colors observed in the arms, which suggests it has relatively low star formation. The galaxy doesn't have any evidence of tidal tails or distortions, suggesting it has not undergone any major mergers recently. The disk appears face-on, giving a clear view of the spiral structure, which appears relatively well-defined despite the galaxy's redshift. There appears to be a weak central bar.