This galaxy exhibits a smooth, elongated morphology, suggestive of an elliptical or lenticular type. The central bulge is prominent, displaying a concentrated, yellowish-white color, potentially indicating an older stellar population. The isophotes appear relatively undisturbed, with no clear evidence of spiral arms or significant tidal features. The galaxy displays a subtle color gradient moving outwards from the bulge, becoming slightly bluer, which could be due to a younger stellar population within a faint disk. The overall structure suggests that the galaxy is nearing the "red and dead" state, with relatively low levels of ongoing star formation.
