This galaxy exhibits an irregular morphology, possibly due to an ongoing or recent interaction. A prominent, bright central region is visible, surrounded by a less defined and somewhat diffuse outer structure. There appears to be a tidal tail emanating from one side of the galaxy, suggesting gravitational disruption. The color distribution indicates a higher concentration of younger, blue stars in the central region and tidal tail. The overall shape deviates significantly from a classical elliptical or spiral form. Some regions show evidence of intense star formation, while others appear more quiescent. The galaxy appears to be undergoing a significant morphological disturbance.
