The galaxy presents as a somewhat diffuse, centrally concentrated object. The overall form appears more akin to a disk galaxy than to an elliptical one. Within the central region, a yellow-orange hue dominates, potentially indicating an older stellar population. Fainter, bluer regions are evident in what could be spiral arms or perhaps disturbed tidal features. The galaxy exhibits a level of asymmetry, possibly due to minor gravitational interactions or internal dynamical processes, though no obvious major merger is apparent. The size appears moderate, extending a few arcseconds across the detector.
