This galaxy appears to be a spiral galaxy, viewed nearly edge-on. A prominent dust lane is not visible. The galaxy exhibits a smooth, elongated profile, with a bright, concentrated central bulge. There are no visible spiral arms, instead there appears to be a disk that has a bluish hue, potentially indicating regions of recent star formation within the galactic disk. The overall structure suggests a relatively low rate of ongoing star formation. There are no obvious signs of major mergers or significant tidal disturbances. The morphology suggests the galaxy is relatively undisturbed, having possibly undergone minor interactions, but is largely stable. The galaxy is of intermediate size and mass.