The galaxy presents a complex morphology, potentially indicative of an ongoing or recent merger event. Two distinct luminous components are observed, each appearing relatively smooth and centrally concentrated. The brighter, lower component exhibits a yellow-red hue. The upper component appears to be similar in color, and is noticeably less bright. A faint bridge of diffuse light seems to connect these two components, suggesting a tidal interaction. The overall shape deviates significantly from a regular elliptical or spiral structure. There are signs of a minor disturbance on one side. The galaxy's color suggests a population of older stars and a lower rate of current star formation.
