The galaxy presents as a relatively smooth, centrally concentrated object. Its overall shape is elliptical, tending towards a somewhat spheroidal morphology. The central region exhibits a bright, yellowish hue, suggesting a population of older, redder stars. Moving outwards from the core, the light gradually fades. There is a hint of a bluish halo surrounding the central bulge, possibly indicating a small amount of younger, bluer stars or a low level of ongoing star formation in the outer regions, though this is very faint. There is no clear evidence of spiral arms or significant dust lanes. It seems relatively undisturbed and possibly not currently undergoing any major mergers.
