The galaxy presents as a disturbed, elongated structure. There is a distinct central bulge with a blueish hue, indicating the presence of relatively young, hot stars. The galaxy appears to be undergoing a merging event, as evidenced by its asymmetrical shape and a potential tidal tail extending from one side. The distribution of light is uneven, with regions of higher concentration in the central area and fainter regions in the outer areas. Overall, the galaxy appears to be an actively evolving system.