This galaxy appears to be a spiral galaxy viewed almost perfectly edge-on. It exhibits a prominent, somewhat boxy bulge, with a significantly extended, thin disk component. There is a notable concentration of light towards the central bulge, which graduates into a diffuse disk. The dust lane appears patchy. The disk's color suggests the presence of a relatively older stellar population and a low star formation rate, with the disk being more populated in older stars. There is no evidence of any ongoing major merger events, though minor disturbances cannot be ruled out. The disk appears smooth, with no discrete features.
