The galaxy presents as a concentrated elliptical morphology. It exhibits a smooth, centrally concentrated light profile with a noticeable absence of spiral arms or distinct features like dust lanes. The core region appears bright and yellowish, suggesting an older stellar population dominating the central area. Moving outward from the core, the light gradually diffuses, transitioning into a faint, more reddish halo. The shape is generally elliptical, with a slight elongation, but it appears largely undisturbed. There is no obvious evidence of ongoing major mergers or tidal interactions. The galaxy's overall color index suggests a mature galaxy, likely with suppressed star formation.
