The galaxy presents a somewhat smooth, elliptical morphology. It has a prominent bulge with a noticeable elongated shape. A significant portion of the light appears concentrated in the central bulge, exhibiting a color gradient that transitions to a bluer hue towards the outer edges. There is no immediately visible evidence of spiral arms or significant dust lanes. Overall, the galaxy exhibits a relatively undisturbed structure with an apparent color profile indicative of ongoing star formation.
