The galaxy exhibits a slightly elongated, disk-like morphology. Its light profile appears relatively smooth, lacking prominent spiral arms or a distinct central bulge. There is a faint suggestion of internal structure, possibly subtle variations in surface brightness across the disk. The galaxy is primarily blue in color, indicating the presence of a younger stellar population. The overall appearance suggests a galaxy that may be undergoing, or has recently undergone, some disturbance, evidenced by possible faint tidal features or irregularities in its shape, though it retains a generally undisturbed morphology. There may be hints of a possible merger event in the past. 
