The galaxy appears to be a spiral galaxy viewed nearly edge-on. A central bulge is visible, exhibiting a smooth, rounded morphology. There is indication of a galactic disk which appears to be relatively thick with no distinct spiral arm structure. There is some evidence of dust obscuration along the galactic plane. The galaxy exhibits a color gradient, with the central bulge appearing more yellow/red and the outer disk displaying a bluer hue. The blue color indicates the presence of some ongoing star formation. There is no apparent major disruption or merging activity.
