The galaxy presents a generally smooth, elliptical morphology. It appears elongated, with a cigar-like shape. The central bulge is prominent and exhibits a yellowish-white hue, indicating an older stellar population. Surrounding the bulge, a fainter disk or halo is visible, displaying a bluish tint, suggestive of younger stars or ongoing star formation. There are no apparent spiral arms or significant dust lanes. The galaxy does not show any signs of major disturbances or mergers, exhibiting a relatively undisturbed structure. The color gradients suggest a radial change in stellar populations, with older stars concentrated towards the center and bluer stars located in the outer regions.
