This galaxy presents as a relatively smooth, elliptical-like structure. The central region exhibits a yellowish hue, potentially indicating an older stellar population and a concentration of evolved stars. Moving outward from the core, a subtle gradient towards bluer colors is observed, possibly suggesting the presence of younger stars in the outer regions, although star formation appears subdued. The overall morphology lacks any distinct spiral arms or significant dust lanes. The galaxy appears moderately elongated, but not highly so. There is no obvious indication of major disturbances or ongoing merger activity, though subtle asymmetries might suggest minor past interactions.
