The galaxy presents a primarily smooth morphology, with a high degree of central concentration. The central bulge is prominent and exhibits a yellowish-white hue, suggesting an older stellar population. The isophotes appear generally elliptical, with a moderate ellipticity. Faint, diffuse extensions are visible along the major axis. A hint of a blueish tint is visible along one edge, which may suggest a region of possible new star formation. Overall, the galaxy's structure is that of a relatively undisturbed system without clear spiral arm features or significant morphological disturbances.
