The galaxy presents as a relatively compact, elliptical-like structure, appearing mostly smooth in texture. Its color is predominantly yellowish-orange, suggesting a population of older stars with lower rates of current star formation. There is a hint of a central concentration of light, but no distinct spiral arms or bar features are discernible. The object has a somewhat rounded appearance, although a slight elongation is observed. Irregularities in the morphology suggest possible minor disturbances or interactions. The galaxy is not completely isolated; what appears to be a smaller object is in very close proximity, potentially indicative of a tidal interaction or an early stage merger. Overall, the image suggests a passively evolving system with ongoing or recent gravitational interactions influencing its morphology.
