The galaxy presents as a relatively smooth, centrally concentrated object. It appears elliptical in shape with a high degree of roundness. The core region exhibits a yellowish hue, suggesting a population of older stars. Surrounding the core, a less defined, diffuse region displays a greenish-blue tint, potentially indicative of more recent star formation, though subdued. No distinct spiral arms or prominent dust lanes are visible, suggesting the absence of a well-defined disk structure. There is no strong evidence of any on-going major merging activity or significant tidal disturbance. The galaxy's overall morphology appears relatively undisturbed and quiescent.
