The galaxy presents as a relatively smooth, elliptical-like structure with a centrally concentrated brightness profile. The core exhibits a strong yellow-orange hue, suggesting an older stellar population and potentially significant dust extinction. The galaxy's light smoothly fades outward from the core, transitioning to a redder color in the outer regions. There is no evidence of spiral arms or distinct features indicative of active star formation, supporting its classification as a passively evolving system. The general morphology suggests it is unlikely to be undergoing any major merging events. It appears fairly isolated with no obvious tidal tails or surrounding companions, although there is a brighter yellow object nearby which may be gravitationally related.
