The galaxy presents a predominantly smooth morphology with minimal discernible features indicative of spiral arms or significant dust lanes. The overall shape appears ellipsoidal, approaching a near-spherical form, though some slight ellipticity can be observed. There is a central concentration of light, suggesting a prominent bulge component. The color profile shifts from a yellowish hue in the core region to a redder tint in the outer regions, potentially indicating an aging stellar population and suppressed star formation in the galaxy's outskirts. The galaxy doesn't show clear signs of ongoing mergers or major tidal disturbances, exhibiting a relatively undisturbed structure.
