The galaxy presents an elongated, cigar-shaped morphology. Its light distribution appears relatively smooth, with a high degree of central concentration. The galaxy exhibits a color gradient, transitioning from a warmer, reddish hue towards the center to a cooler, bluish tint at its periphery. There is no immediately discernible spiral structure or prominent dust lanes. The overall light profile suggests a quiescent galaxy with possible recent or ongoing star formation contributing to the bluer edges. There are no obvious signs of major interactions or mergers, although a minor disturbance cannot be completely ruled out based on this image.
