The galaxy presents as an elongated structure with a bright, concentrated central bulge. The bulge exhibits a yellowish-white color, suggesting an older stellar population. Extending from the central bulge is a fainter, somewhat diffuse disk. The disk appears to be oriented edge-on or nearly edge-on, and shows hints of structure, but is not fully resolved. The color gradient from the bulge to the outer disk suggests some ongoing star formation. There are subtle indications of minor tidal disturbances or asymmetries in the outer regions of the disk, but overall the galaxy appears relatively undisturbed.
