The galaxy presents a generally smooth, elliptical morphology. It appears to be largely spheroidal, with a high degree of central concentration of light. There is a prominent central bulge region which emits strongly in the observed visual bands, transitioning into a more diffuse halo. The color profile suggests the presence of a stellar population that skews older, as evidenced by the reddish-yellow hue of the central region, potentially indicative of evolved stars. There's a lack of distinct spiral arm structures or prominent dust lanes. The galaxy appears relatively undisturbed, showing no obvious signs of ongoing major mergers or significant tidal interactions. There may be subtle indications of possible minor disturbances in the outer regions.
