The galaxy presents as a relatively luminous, disk-shaped structure oriented at a significant inclination to our line of sight. The central region exhibits a pronounced bulge, appearing smooth and concentrated with a yellowish-white hue, suggestive of an older stellar population. A fainter, bluer disk surrounds the central bulge, indicating the presence of younger, hotter stars and possibly some ongoing star formation. The overall morphology appears relatively undisturbed, with no obvious signs of major mergers or significant tidal features. There is a hint of dust lane obscuration along the major axis on one side of the bulge. The outer regions of the disk show subtle irregularities and a decrease in surface brightness. The galaxy's elongated shape suggests a moderate degree of flattening.
