The galaxy presents a somewhat amorphous structure. Its overall color profile trends towards a blue hue, indicating a population of relatively young, hot stars. The light is somewhat diffused, making the boundary of the galaxy difficult to define precisely. There are no prominent spiral arm structures visible. Instead, there is a nebulous glow with what appears to be some clumpy regions, potentially areas of active star formation. The morphology suggests a possible merger event with mild tidal disturbances, marked by subtle asymmetries and an overall irregular shape. No clear central bulge is discernible, but there is a brighter area within the diffused light, suggesting a higher concentration of stars in the galaxy's core. There appears to be a slight perturbation to one side, hinting at possible ongoing interaction with a companion galaxy or past gravitational disruption.
