The galaxy presents a generally smooth, elliptical morphology, elongated in shape. The central bulge exhibits a concentration of older stars, indicated by its yellowish-orange hue. Surrounding the bulge, there's a fainter, bluish-white disk component, possibly suggesting ongoing star formation. There appear to be no prominent spiral arms or bar structures. There's no evidence of any major mergers or significant tidal disturbances affecting the galaxy's structure, suggesting it is relatively undisturbed. The galaxy's color gradients imply a higher concentration of older stellar populations in the core, transitioning to younger populations in the outer regions of the disk.
