The galaxy presents a morphology suggestive of a system undergoing interaction or merging activity. Its overall shape is elongated, and the light distribution appears disturbed, lacking a well-defined spiral or elliptical structure. There is a brighter central concentration of light. One area is more diffuse and somewhat distorted, possibly indicative of tidal features or ongoing accretion. Patches of bluer light are observed, suggesting regions of active star formation, while the remaining areas exhibit a more yellow/orange color.
