The galaxy presents as a smooth, centrally concentrated object with a generally elliptical morphology. The central bulge region exhibits a bright, yellowish hue, suggestive of an older stellar population. There is a subtle color gradient from the center outwards, with the outer regions appearing slightly bluer. There is no clear evidence of spiral arm structure or significant dust lanes. The smooth profile and lack of distinct features indicate a relatively undisturbed system, with possible low ongoing star formation.
