This galaxy presents as a disk galaxy, seen nearly edge-on. The galaxy appears to be dominated by an elliptical bulge, centrally located. The bulge exhibits a smooth, homogenous texture with an orange hue, possibly indicating an older stellar population. The disk component is visible as fainter, bluer light extending outwards from the central bulge, tapering off at the edges. The disk appears relatively thin. Little to no dust lanes or active star formation regions are discernible. The galaxy exhibits a low star formation rate, indicating that it is relatively quiescent. There is no evidence of significant tidal disturbances or ongoing mergers. The morphology suggests a well-evolved, relatively undisturbed system.
