The galaxy appears to be a relatively smooth, centrally concentrated object. Its morphology suggests an elliptical or lenticular galaxy classification, exhibiting a spheroidal shape with a lack of distinct spiral arms. A subtle color gradient is observable, with a slightly bluer hue in the central region, transitioning to redder tones in the outer halo, potentially indicative of varying stellar populations. The overall structure suggests a system dominated by older stars. There is no evident active galactic nucleus or significant dust lanes. No major mergers or tidal disturbances are visible, suggesting a relaxed and relatively undisturbed system. The galaxy displays a fairly high degree of central concentration, with the majority of the light emanating from a compact core.